This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.66 01:56:38.09 +59:15:33.9
131.18816 -2.56322 galactic Cas Second-epoch detections are separated by 0.6" and 7.8 pix
The object was found in VSX 0" X Cas
Type: M
# Max. Min./Amp. JD0 Period
9.450 V 13.200 V 2457020.00000 415.000000000000 C5,4e(N1e)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.09 +59:15:33.9: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.09 +59:15:33.9: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 56 38.09 +59 15 33.9 8.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
X Cas,2461199.8322,8.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
X Cas 20260608.3322 8.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 11.14 01:16:28.97 +60:14:00.3
126.03868 -2.48717 galactic Cas Second-epoch detections are separated by 1.5" and 7.0 pix
The object was found in ASASSN-V 1" ASASSN-V J011628.82+601400.9
Type: SR
MeanMag 13.24 m Amp. 0.36 m Period 128.0 d
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:28.97 +60:14:00.3: 14.73 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:28.97 +60:14:00.3: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 16 28.97 +60 14 00.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461199.8322,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260608.3322 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.80 02:24:29.85 +59:24:31.1
134.53129 -1.35104 galactic Cas Second-epoch detections are separated by 1.1" and 8.3 pix
The object was found in VSX 1" V0672 Cas
Type: SR
# Max. Min./Amp. JD0 Period
15.000 B 17.400 B 302.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:29.85 +59:24:31.1: 15.67 +/- 0.31 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:29.85 +59:24:31.1: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 29.85 +59 24 31.1 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0672 Cas,2461199.8322,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0672 Cas 20260608.3322 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.43 02:21:40.72 +60:54:41.9
133.68147 -0.06269 galactic Cas Second-epoch detections are separated by 0.5" and 8.2 pix
The object was found in VSX 1" DE Cas
Type: SRB
# Max. Min./Amp. JD0 Period
13.900 pg 15.100 pg 2428925.00000 151.000000000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:40.72 +60:54:41.9: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:40.72 +60:54:41.9: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 40.72 +60 54 41.9 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DE Cas,2461199.8322,9.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DE Cas 20260608.3322 9.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.88 02:28:33.48 +62:03:22.8
134.04450 1.29834 galactic Cas Second-epoch detections are separated by 2.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:28:33.48 +62:03:22.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:33.48 +62:03:22.8: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:33.48 +62:03:22.8: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 28 33.48 +62 03 22.8 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.68 02:52:02.80 +63:39:30.2
135.83987 3.85101 galactic Cas Second-epoch detections are separated by 5.4" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:52:02.80 +63:39:30.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:52:02.80 +63:39:30.2: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:52:02.80 +63:39:30.2: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 52 02.80 +63 39 30.2 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.96 01:59:42.41 +63:32:29.7
130.44896 1.67061 galactic Cas Second-epoch detections are separated by 3.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:59:42.41 +63:32:29.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:42.41 +63:32:29.7: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:42.41 +63:32:29.7: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 59 42.41 +63 32 29.7 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.86 02:14:53.05 +64:11:56.5
131.85910 2.78324 galactic Cas Second-epoch detections are separated by 1.9" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:14:53.05 +64:11:56.5 (user input) | T | P | (position from user input) J-Ks=0.807+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:14:53.05 +64:11:56.5: 12.14 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:14:53.05 +64:11:56.5: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 14 53.05 +64 11 56.5 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.78 02:08:06.43 +63:06:02.0
131.47746 1.50791 galactic Cas Second-epoch detections are separated by 4.0" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:08:06.43 +63:06:02.0 (user input) | T | P | (position from user input) J-Ks=0.615+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:08:06.43 +63:06:02.0: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:08:06.43 +63:06:02.0: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 08 06.43 +63 06 02.0 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.94 01:13:39.59 +63:12:31.2
125.43296 0.44488 galactic Cas Second-epoch detections are separated by 4.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:13:39.59 +63:12:31.2 (user input) | T | P | (position from user input) J-Ks=1.187+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:39.59 +63:12:31.2: 12.60 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:39.59 +63:12:31.2: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 13 39.59 +63 12 31.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.56 01:00:19.87 +57:17:48.3
124.13860 -5.55416 galactic Cas Second-epoch detections are separated by 1.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:00:19.87 +57:17:48.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:00:19.87 +57:17:48.3: 12.63 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:00:19.87 +57:17:48.3: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 00 19.87 +57 17 48.3 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.67 00:46:00.34 +57:56:20.1
122.20840 -4.92520 galactic Cas Second-epoch detections are separated by 5.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:46:00.34 +57:56:20.1 (user input) | T | P | (position from user input) J-Ks=0.885+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:46:00.34 +57:56:20.1: 11.65 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:46:00.34 +57:56:20.1: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 00 46 00.34 +57 56 20.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.71 00:37:39.91 +62:15:59.9
121.33028 -0.56227 galactic Cas Second-epoch detections are separated by 4.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:37:39.91 +62:15:59.9 (user input) | T | P | (position from user input) J-Ks=0.849+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:37:39.91 +62:15:59.9: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:37:39.91 +62:15:59.9: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 00 37 39.91 +62 15 59.9 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.38 01:02:20.28 +57:02:48.2
124.42142 -5.79350 galactic Cas Second-epoch detections are separated by 1.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J015.5833+57.0370 | 01:02:20.28 +57:02:48.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.376+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:02:20.28 +57:02:48.2: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:02:20.28 +57:02:48.2: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 02 20.28 +57 02 48.2 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J015.5833+57.0370,2461199.8322,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J015.5833+57.0370 20260608.3322 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.71 01:08:39.11 +60:32:48.4
125.04812 -2.25422 galactic Cas Second-epoch detections are separated by 1.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:08:39.11 +60:32:48.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:39.11 +60:32:48.4: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:39.11 +60:32:48.4: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 08 39.11 +60 32 48.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.80 01:19:04.47 +60:02:34.1
126.37941 -2.64382 galactic Cas Second-epoch detections are separated by 1.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:19:04.47 +60:02:34.1 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:04.47 +60:02:34.1: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:04.47 +60:02:34.1: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 19 04.47 +60 02 34.1 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.63 00:47:54.55 +59:03:26.0
122.47732 -3.81141 galactic Cas Second-epoch detections are separated by 1.8" and 6.2 pix
The object was found in VSX19" Gaia DR3 425228395406329088
Type: E
# Max. Min./Amp. JD0 Period
16.000 G 16.210 G 11.110700000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:47:54.55 +59:03:26.0: 11.38 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:47:54.55 +59:03:26.0: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 00 47 54.55 +59 03 26.0 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 425228395406329088,2461199.8322,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 425228395406329088 20260608.3322 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.43 01:42:54.46 +61:13:30.6
129.08679 -1.03000 galactic Cas Second-epoch detections are separated by 2.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:42:54.46 +61:13:30.6 (user input) | T | P | (position from user input) J-Ks=0.763+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:42:54.46 +61:13:30.6: 10.67 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:42:54.46 +61:13:30.6: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 42 54.46 +61 13 30.6 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.29 02:52:09.97 +62:49:57.4
136.22261 3.11880 galactic Cas Second-epoch detections are separated by 6.2" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:52:09.97 +62:49:57.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:52:09.97 +62:49:57.4: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:52:09.97 +62:49:57.4: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 52 09.97 +62 49 57.4 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.95 02:27:39.78 +57:06:42.3
135.74224 -3.34729 galactic Per Second-epoch detections are separated by 6.0" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.8997+57.1175 | 02:27:35.93 +57:07:03.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:39.78 +57:06:42.3: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:39.78 +57:06:42.3: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 39.78 +57 06 42.3 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.8997+57.1175,2461199.8322,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.8997+57.1175 20260608.3322 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.38 02:30:58.90 +62:01:46.4
134.31835 1.37866 galactic Cas Second-epoch detections are separated by 8.0" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:30:58.90 +62:01:46.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:58.90 +62:01:46.4: 12.82 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:58.90 +62:01:46.4: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 58.90 +62 01 46.4 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.45 01:17:48.39 +57:17:35.2
126.50421 -5.39563 galactic Cas Second-epoch detections are separated by 2.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:17:48.39 +57:17:35.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:48.39 +57:17:35.2: 12.99 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:48.39 +57:17:35.2: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 17 48.39 +57 17 35.2 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.26 01:57:25.08 +60:33:52.9
130.95490 -1.27519 galactic Cas Second-epoch detections are separated by 5.3" and 7.8 pix
The object was found in VSX17" Gaia DR3 508205411215994240
Type: VAR
# Max. Min./Amp. JD0 Period
13.480 G 13.550 G 0.554370000000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:25.08 +60:33:52.9: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:25.08 +60:33:52.9: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 57 25.08 +60 33 52.9 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508205411215994240,2461199.8322,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508205411215994240 20260608.3322 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.21 02:28:28.47 +58:25:05.6
135.36618 -2.09131 galactic Per Second-epoch detections are separated by 8.0" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458872832740545280 | 02:28:28.03 +58:25:04.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:28.47 +58:25:05.6: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:28.47 +58:25:05.6: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 28 28.47 +58 25 05.6 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458872832740545280,2461199.8322,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458872832740545280 20260608.3322 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.45 02:37:12.84 +63:10:37.8
134.53732 2.71392 galactic Cas Second-epoch detections are separated by 7.4" and 8.3 pix
The object was found in VSX13" Gaia DR3 514150676749706240
Type: ROT
# Max. Min./Amp. JD0 Period
15.930 G 15.980 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:12.84 +63:10:37.8: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:12.84 +63:10:37.8: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 37 12.84 +63 10 37.8 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 514150676749706240,2461199.8322,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 514150676749706240 20260608.3322 10.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.26 00:55:16.01 +57:59:06.5
123.44121 -4.88282 galactic Cas Second-epoch detections are separated by 3.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J013.8119+57.9861 | 00:55:16.01 +57:59:06.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.410+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:55:16.01 +57:59:06.5: 11.25 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:55:16.01 +57:59:06.5: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 00 55 16.01 +57 59 06.5 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J013.8119+57.9861,2461199.8322,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J013.8119+57.9861 20260608.3322 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.53 00:56:47.59 +60:38:47.2
123.58865 -2.21848 galactic Cas Second-epoch detections are separated by 3.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 426546125736902528 | 00:56:44.52 +60:38:23.6 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:56:47.59 +60:38:47.2: 10.80 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:56:47.59 +60:38:47.2: 13.34 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 00 56 47.59 +60 38 47.2 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426546125736902528,2461199.8322,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426546125736902528 20260608.3322 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.41 02:01:32.89 +65:05:48.8
130.22916 3.22319 galactic Cas Second-epoch detections are separated by 1.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:01:32.89 +65:05:48.8 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.029 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:32.89 +65:05:48.8: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:32.89 +65:05:48.8: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 01 32.89 +65 05 48.8 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.91 01:59:56.21 +56:37:09.2
132.29136 -5.00264 galactic Per Second-epoch detections are separated by 2.8" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J029.9925+56.6233 | 01:59:56.21 +56:37:09.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.461+/-0.181 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:56.21 +56:37:09.2: 11.80 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:56.21 +56:37:09.2: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 59 56.21 +56 37 09.2 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J029.9925+56.6233,2461199.8322,9.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J029.9925+56.6233 20260608.3322 9.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.04 01:08:29.49 +57:06:54.4
125.25665 -5.67964 galactic Cas Second-epoch detections are separated by 6.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:08:29.49 +57:06:54.4 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:29.49 +57:06:54.4: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:29.49 +57:06:54.4: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 08 29.49 +57 06 54.4 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.31 00:52:55.06 +58:28:52.6
123.12588 -4.38991 galactic Cas Second-epoch detections are separated by 6.0" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J013.2201+58.4812 | 00:52:55.06 +58:28:52.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:55.06 +58:28:52.6: 11.23 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:55.06 +58:28:52.6: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 00 52 55.06 +58 28 52.6 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J013.2201+58.4812,2461199.8322,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J013.2201+58.4812 20260608.3322 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.79 02:17:47.56 +56:14:45.2
134.76773 -4.62855 galactic Per Second-epoch detections are separated by 4.4" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J034.4495+56.2466 | 02:17:44.71 +56:15:01.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:17:47.56 +56:14:45.2: 13.05 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:17:47.56 +56:14:45.2: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 17 47.56 +56 14 45.2 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J034.4495+56.2466,2461199.8322,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J034.4495+56.2466 20260608.3322 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.66 02:36:02.71 +59:00:55.3
136.04945 -1.16619 galactic Cas Second-epoch detections are separated by 3.1" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.0107+59.0168 | 02:36:02.57 +59:01:00.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:02.71 +59:00:55.3: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:02.71 +59:00:55.3: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 36 02.71 +59 00 55.3 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.0107+59.0168,2461199.8322,9.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.0107+59.0168 20260608.3322 9.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.73 02:25:54.13 +56:38:48.5
135.68532 -3.86767 galactic Per Second-epoch detections are separated by 0.7" and 8.4 pix
The object was found in VSX16" Gaia DR3 457634404691160448
Type: RS
# Max. Min./Amp. JD0 Period
17.620 G 17.730 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:54.13 +56:38:48.5: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:54.13 +56:38:48.5: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 54.13 +56 38 48.5 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457634404691160448,2461199.8322,9.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457634404691160448 20260608.3322 9.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.09 02:18:52.86 +63:06:09.6
132.63494 1.89010 galactic Cas Second-epoch detections are separated by 1.1" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 513961148433851008 | 02:18:52.81 +63:06:09.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.729+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:52.86 +63:06:09.6: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:52.86 +63:06:09.6: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 18 52.86 +63 06 09.6 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 513961148433851008,2461199.8322,10.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 513961148433851008 20260608.3322 10.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.63 00:30:29.66 +66:05:42.3
120.80915 3.30969 galactic Cas Second-epoch detections are separated by 3.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:30:29.66 +66:05:42.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:30:29.66 +66:05:42.3: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:30:29.66 +66:05:42.3: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 00 30 29.66 +66 05 42.3 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.77 02:19:40.58 +56:48:52.6
134.82419 -4.00588 galactic Per Second-epoch detections are separated by 1.1" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458351904751297280 | 02:19:38.26 +56:49:13.9 (Gaia DR3) | DSCT/GDOR (local) | B (local) | Gaia3var=VARIABLE J-Ks=-0.005+/-0.042 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:40.58 +56:48:52.6: 12.96 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:40.58 +56:48:52.6: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 19 40.58 +56 48 52.6 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458351904751297280,2461199.8322,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458351904751297280 20260608.3322 9.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.22 01:25:15.63 +64:40:33.5
126.54027 2.04145 galactic Cas Second-epoch detections are separated by 4.3" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 512840196327698304 | 01:25:16.38 +64:40:51.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:15.63 +64:40:33.5: 11.18 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:15.63 +64:40:33.5: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 25 15.63 +64 40 33.5 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512840196327698304,2461199.8322,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512840196327698304 20260608.3322 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.21 00:46:11.73 +59:43:33.6
122.27024 -3.13901 galactic Cas Second-epoch detections are separated by 4.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:46:11.73 +59:43:33.6 (user input) | T | P | (position from user input) J-Ks=1.303+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:46:11.73 +59:43:33.6: 10.86 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:46:11.73 +59:43:33.6: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 00 46 11.73 +59 43 33.6 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.61 02:19:45.01 +56:50:30.5
134.82459 -3.97687 galactic Per Second-epoch detections are separated by 0.6" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458353485299237632 | 02:19:41.57 +56:50:54.7 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.050+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:45.01 +56:50:30.5: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:45.01 +56:50:30.5: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 19 45.01 +56 50 30.5 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458353485299237632,2461199.8322,9.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458353485299237632 20260608.3322 9.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.71 02:20:35.00 +57:06:52.7
134.83962 -3.68175 galactic Per Second-epoch detections are separated by 6.9" and 7.5 pix
The object was found in VSX 4" Gaia DR3 458363071665935616
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.250 G 12.310 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:35.00 +57:06:52.7: 12.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:35.00 +57:06:52.7: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 20 35.00 +57 06 52.7 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458363071665935616,2461199.8322,9.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458363071665935616 20260608.3322 9.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.05 02:00:17.31 +65:03:54.9
130.10949 3.15738 galactic Cas Second-epoch detections are separated by 2.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 518142144475250304 | 02:00:13.19 +65:04:05.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:17.31 +65:03:54.9: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:17.31 +65:03:54.9: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 00 17.31 +65 03 54.9 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 518142144475250304,2461199.8322,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 518142144475250304 20260608.3322 10.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.62 02:20:50.58 +57:20:41.9
134.79459 -3.45313 galactic Per Second-epoch detections are separated by 3.6" and 8.6 pix
The object was found in VSX 4" Gaia DR3 458472296969558272
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.290 G 12.310 G 0.081775600000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:50.58 +57:20:41.9: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:50.58 +57:20:41.9: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 20 50.58 +57 20 41.9 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458472296969558272,2461199.8322,9.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458472296969558272 20260608.3322 9.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.37 01:43:21.66 +56:52:28.8
130.01302 -5.28151 galactic Cas Second-epoch detections are separated by 1.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 505817439459624832 | 01:43:21.55 +56:52:24.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:21.66 +56:52:28.8: 12.94 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:21.66 +56:52:28.8: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 43 21.66 +56 52 28.8 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 505817439459624832,2461199.8322,9.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505817439459624832 20260608.3322 9.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.68 00:36:54.99 +62:40:45.5
121.26657 -0.14548 galactic Cas Second-epoch detections are separated by 4.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 430706329831264640 | 00:36:57.75 +62:40:57.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:36:54.99 +62:40:45.5: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:36:54.99 +62:40:45.5: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 00 36 54.99 +62 40 45.5 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 430706329831264640,2461199.8322,9.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430706329831264640 20260608.3322 9.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.72 02:19:45.19 +57:01:14.5
134.76485 -3.80820 galactic Per Second-epoch detections are separated by 1.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458361216240219648 | 02:19:47.59 +57:00:57.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:45.19 +57:01:14.5: 12.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:45.19 +57:01:14.5: 11.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 19 45.19 +57 01 14.5 8.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458361216240219648,2461199.8322,8.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458361216240219648 20260608.3322 8.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 6.68 02:29:09.04 +56:37:12.3
136.11213 -3.73038 galactic Per Second-epoch detections are separated by 0.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 457593928911905280 | 02:29:09.04 +56:37:12.3 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: A0V 1966POHP....8...25F BD+55 629 J-Ks=0.123+/-0.029 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:09.04 +56:37:12.3: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:09.04 +56:37:12.3: 9.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.24 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 09.04 +56 37 12.3 6.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 457593928911905280,2461199.8322,6.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 457593928911905280 20260608.3322 6.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 6.79 02:25:27.60 +56:46:56.1
135.58011 -3.76276 galactic Per Second-epoch detections are separated by 0.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.3787+56.7792 | 02:25:27.69 +56:46:54.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.194+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:27.60 +56:46:56.1: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:27.60 +56:46:56.1: 9.69 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.69 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 27.60 +56 46 56.1 6.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.3787+56.7792,2461199.8322,6.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.3787+56.7792 20260608.3322 6.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 6.96 02:34:10.54 +55:50:00.3
137.05819 -4.19486 galactic Per Second-epoch detections are separated by 9.3" and 8.5 pix
The object was found in VSX 5" Gaia DR3 457311320070532608
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
9.230 G 9.290 G 0.086248700000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:10.54 +55:50:00.3: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:10.54 +55:50:00.3: 9.49 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.49 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 10.54 +55 50 00.3 7.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457311320070532608,2461199.8322,6.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457311320070532608 20260608.3322 6.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 6.98 02:23:38.00 +56:52:44.8
135.31158 -3.76017 galactic Per Second-epoch detections are separated by 0.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458388978906447488 | 02:23:37.93 +56:52:45.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 2002ApJ...576..880S [SHM2002] 59 J-Ks=0.318+/-0.036 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:38.00 +56:52:44.8: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:38.00 +56:52:44.8: 9.56 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.56 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 38.00 +56 52 44.8 7.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458388978906447488,2461199.8322,6.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458388978906447488 20260608.3322 6.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 6.98 02:22:03.76 +56:31:27.4
135.23211 -4.16772 galactic Per Second-epoch detections are separated by 0.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.5283+56.5245 | 02:22:03.76 +56:31:27.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.139+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:03.76 +56:31:27.4: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:03.76 +56:31:27.4: 9.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.52 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 03.76 +56 31 27.4 7.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.5283+56.5245,2461199.8322,6.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.5283+56.5245 20260608.3322 6.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 6.91 02:32:34.58 +57:29:15.3
136.21908 -2.75158 galactic Per Second-epoch detections are separated by 0.7" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458019817868936448 | 02:32:34.57 +57:29:15.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.631+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:34.58 +57:29:15.3: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:34.58 +57:29:15.3: 9.45 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.45 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 34.58 +57 29 15.3 6.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458019817868936448,2461199.8322,6.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458019817868936448 20260608.3322 6.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 6.88 02:34:00.78 +57:49:58.1
136.26438 -2.35910 galactic Per Second-epoch detections are separated by 1.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.5124+57.8270 | 02:34:00.89 +57:49:57.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.860+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:00.78 +57:49:58.1: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:00.78 +57:49:58.1: 9.49 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.49 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 00.78 +57 49 58.1 6.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.5124+57.8270,2461199.8322,6.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.5124+57.8270 20260608.3322 6.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.11 02:25:20.48 +56:51:13.6
135.53942 -3.70167 galactic Per Second-epoch detections are separated by 1.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457640417645156608 | 02:25:20.39 +56:51:13.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB- 1959LS....C01....0H LS I +56 49 J-Ks=0.067+/-0.030 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:20.48 +56:51:13.6: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:20.48 +56:51:13.6: 9.67 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.67 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 20.48 +56 51 13.6 7.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457640417645156608,2461199.8322,7.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457640417645156608 20260608.3322 7.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.00 02:29:10.13 +56:27:12.4
136.17608 -3.88435 galactic Per Second-epoch detections are separated by 2.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457590355506120064 | 02:29:10.50 +56:27:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:10.13 +56:27:12.4: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:10.13 +56:27:12.4: 9.57 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.57 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 10.13 +56 27 12.4 7.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457590355506120064,2461199.8322,7.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457590355506120064 20260608.3322 7.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.06 02:35:37.82 +57:29:13.2
136.59830 -2.59376 galactic Per Second-epoch detections are separated by 0.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458101181736200448 | 02:35:37.84 +57:29:13.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1928AnHar.100...49C HD 236971 J-Ks=0.171+/-0.037 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:37.82 +57:29:13.2: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:37.82 +57:29:13.2: 9.60 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.60 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 35 37.82 +57 29 13.2 7.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458101181736200448,2461199.8322,7.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458101181736200448 20260608.3322 7.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.12 02:27:24.37 +56:23:03.5
135.97405 -4.03787 galactic Per Second-epoch detections are separated by 0.8" and 8.5 pix
The object was found in VSX 1" Gaia DR3 457563554909169536
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
9.480 G 9.530 G 0.595500000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:24.37 +56:23:03.5: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:24.37 +56:23:03.5: 9.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.59 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 24.37 +56 23 03.5 7.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457563554909169536,2461199.8322,7.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457563554909169536 20260608.3322 7.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.20 02:23:35.48 +56:34:27.4
135.41286 -4.04783 galactic Per Second-epoch detections are separated by 1.0" and 8.4 pix
The object was found in VSX 1" V0361 Per
Type: GCAS
# Max. Min./Amp. JD0 Period
9.060 V 9.640 V B1.5IIIpe
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:35.48 +56:34:27.4: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:35.48 +56:34:27.4: 9.50 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.50 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 35.48 +56 34 27.4 7.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0361 Per,2461199.8322,7.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0361 Per 20260608.3322 7.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.15 02:34:44.20 +56:06:07.0
137.02636 -3.91690 galactic Per Second-epoch detections are separated by 7.0" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.6785+56.0961 | 02:34:44.47 +56:06:09.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:44.20 +56:06:07.0: 12.26 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:44.20 +56:06:07.0: 9.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.70 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 44.20 +56 06 07.0 7.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.6785+56.0961,2461199.8322,7.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.6785+56.0961 20260608.3322 7.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.23 02:24:11.88 +56:35:43.2
135.48389 -3.99886 galactic Per Second-epoch detections are separated by 0.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457537269710765824 | 02:24:11.89 +56:35:43.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1966POHP....8...25F BD+55 607 J-Ks=0.116+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:11.88 +56:35:43.2: 8.76 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:11.88 +56:35:43.2: 9.77 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.73 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 11.88 +56 35 43.2 7.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457537269710765824,2461199.8322,7.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457537269710765824 20260608.3322 7.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.19 02:33:34.76 +55:54:25.0
136.95237 -4.15928 galactic Per Second-epoch detections are separated by 6.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.3939+55.9184 | 02:33:35.02 +55:54:27.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:34.76 +55:54:25.0: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:34.76 +55:54:25.0: 9.69 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.69 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 34.76 +55 54 25.0 7.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.3939+55.9184,2461199.8322,7.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.3939+55.9184 20260608.3322 7.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.10 02:31:26.00 +55:59:07.0
136.64394 -4.20129 galactic Per Second-epoch detections are separated by 4.6" and 8.5 pix
The object was found in VSX21" Gaia DR3 457343205908261760
Type: ROT
# Max. Min./Amp. JD0 Period
16.250 G 16.350 G 0.771500000000 M
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:26.00 +55:59:07.0: 12.78 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:26.00 +55:59:07.0: 9.44 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.44 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 26.00 +55 59 07.0 7.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457343205908261760,2461199.8322,7.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457343205908261760 20260608.3322 7.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.42 02:18:01.26 +56:15:41.5
134.79262 -4.60335 galactic Per Second-epoch detections are separated by 1.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 456810595604427392 | 02:18:01.38 +56:15:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 2013AJ....145..102L PM J02180+5616 J-Ks=1.098+/-0.040 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:01.26 +56:15:41.5: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:01.26 +56:15:41.5: 10.22 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.22 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 18 01.26 +56 15 41.5 7.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 456810595604427392,2461199.8322,7.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 456810595604427392 20260608.3322 7.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.38 02:36:36.22 +57:46:58.9
136.60179 -2.27036 galactic Cas Second-epoch detections are separated by 0.9" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx3855710 | 02:36:36.18 +57:46:59.2 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE SpType: A0 1928AnHar.100...49C HD 236973 J-Ks=0.098+/-0.028 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:36.22 +57:46:58.9: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:36.22 +57:46:58.9: 9.93 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.93 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 36 36.22 +57 46 58.9 7.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3855710,2461199.8322,7.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3855710 20260608.3322 7.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.42 02:19:46.68 +56:22:26.5
134.98555 -4.41626 galactic Per Second-epoch detections are separated by 0.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458272121436434944 | 02:19:46.67 +56:22:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.132+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:46.68 +56:22:26.5: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:46.68 +56:22:26.5: 10.03 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.03 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 19 46.68 +56 22 26.5 7.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458272121436434944,2461199.8322,7.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458272121436434944 20260608.3322 7.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.37 02:35:52.03 +57:47:22.2
136.50893 -2.30301 galactic Cas Second-epoch detections are separated by 0.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458114582034037760 | 02:35:52.03 +57:47:22.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB 1953BOTT....1g...3G BD+57 593 J-Ks=0.224+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:52.03 +57:47:22.2: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:52.03 +57:47:22.2: 9.95 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.95 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 35 52.03 +57 47 22.2 7.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458114582034037760,2461199.8322,7.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458114582034037760 20260608.3322 7.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.38 02:23:26.41 +56:06:42.3
135.55505 -4.48859 galactic Per Second-epoch detections are separated by 2.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457520296000263808 | 02:23:26.45 +56:06:41.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.676+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:26.41 +56:06:42.3: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:26.41 +56:06:42.3: 10.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.06 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 26.41 +56 06 42.3 7.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457520296000263808,2461199.8322,7.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457520296000263808 20260608.3322 7.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.39 02:36:33.27 +57:54:38.9
136.54534 -2.15552 galactic Cas Second-epoch detections are separated by 0.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:36:33.27 +57:54:38.9 (user input) | T | P | (position from user input) J-Ks=0.899+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:33.27 +57:54:38.9: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:33.27 +57:54:38.9: 10.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.13 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 36 33.27 +57 54 38.9 7.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,7.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 7.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.48 02:21:55.20 +56:25:08.5
135.24981 -4.27333 galactic Per Second-epoch detections are separated by 0.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458281467286227200 | 02:21:55.21 +56:25:08.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.079+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:55.20 +56:25:08.5: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:55.20 +56:25:08.5: 10.00 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.00 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 55.20 +56 25 08.5 7.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458281467286227200,2461199.8322,7.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458281467286227200 20260608.3322 7.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.54 02:21:50.33 +56:34:31.6
135.18545 -4.13025 galactic Per Second-epoch detections are separated by 0.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458284662741800064 | 02:21:50.31 +56:34:32.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB- 1965LS....C05....0H LS V +56 35 J-Ks=0.027+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:50.33 +56:34:31.6: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:50.33 +56:34:31.6: 10.08 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.08 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 50.33 +56 34 31.6 7.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458284662741800064,2461199.8322,7.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458284662741800064 20260608.3322 7.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.60 02:20:54.08 +56:16:37.4
135.16540 -4.45496 galactic Per Second-epoch detections are separated by 1.7" and 8.4 pix
The object was found in VSX 3" ASASSN-V J022054.22+561634.7
Type: SRS
# Max. Min./Amp. JD0 Period
10.990 V 11.120 V 2457360.93000 22.473000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:54.08 +56:16:37.4: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:54.08 +56:16:37.4: 10.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.70 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 20 54.08 +56 16 37.4 7.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J022054.22+561634.7,2461199.8322,7.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J022054.22+561634.7 20260608.3322 7.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.61 02:22:35.38 +56:18:13.9
135.37690 -4.34950 galactic Per Second-epoch detections are separated by 1.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458276622563145984 | 02:22:35.42 +56:18:12.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.639+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:35.38 +56:18:13.9: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:35.38 +56:18:13.9: 10.31 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.31 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 35.38 +56 18 13.9 7.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458276622563145984,2461199.8322,7.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458276622563145984 20260608.3322 7.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.54 02:34:44.93 +57:54:58.3
136.32238 -2.24436 galactic Per Second-epoch detections are separated by 1.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458131487024783872 | 02:34:45.08 +57:54:57.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.066+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:44.93 +57:54:58.3: 13.23 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:44.93 +57:54:58.3: 10.28 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.28 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 44.93 +57 54 58.3 7.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458131487024783872,2461199.8322,7.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458131487024783872 20260608.3322 7.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.57 02:30:44.95 +56:56:12.6
136.19787 -3.35496 galactic Per Second-epoch detections are separated by 0.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.6828+56.9432 | 02:30:44.89 +56:56:12.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.356+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:44.95 +56:56:12.6: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:44.95 +56:56:12.6: 10.12 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.12 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 44.95 +56 56 12.6 7.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.6828+56.9432,2461199.8322,7.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.6828+56.9432 20260608.3322 7.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.54 02:32:05.73 +57:22:03.4
136.20475 -2.88714 galactic Per Second-epoch detections are separated by 1.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.0242+57.3766 | 02:32:05.82 +57:22:02.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.053+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:05.73 +57:22:03.4: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:05.73 +57:22:03.4: 10.20 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.20 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 05.73 +57 22 03.4 7.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.0242+57.3766,2461199.8322,7.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.0242+57.3766 20260608.3322 7.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.79 02:21:20.53 +56:29:12.7
135.15131 -4.23691 galactic Per Second-epoch detections are separated by 0.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458294214749131648 | 02:21:20.46 +56:29:12.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.785+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:20.53 +56:29:12.7: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:20.53 +56:29:12.7: 10.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.59 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 20.53 +56 29 12.7 7.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458294214749131648,2461199.8322,7.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458294214749131648 20260608.3322 7.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.77 02:24:43.66 +56:59:33.7
135.41166 -3.60141 galactic Per Second-epoch detections are separated by 0.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:24:43.66 +56:59:33.7 (user input) | T | P | (position from user input) J-Ks=-0.015+/-0.033 (B)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:43.66 +56:59:33.7: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:43.66 +56:59:33.7: 10.30 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.30 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 43.66 +56 59 33.7 7.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,7.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 7.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.75 02:22:06.90 +56:07:52.9
135.37446 -4.53417 galactic Per Second-epoch detections are separated by 0.5" and 8.4 pix
The object was found in VSX 1" V0758 Per
Type: EA
# Max. Min./Amp. JD0 Period
10.600 R1 10.900 R1 2451450.61000 5.675130000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:06.90 +56:07:52.9: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:06.90 +56:07:52.9: 10.48 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.48 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 06.90 +56 07 52.9 7.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0758 Per,2461199.8322,7.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0758 Per 20260608.3322 7.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.75 02:37:36.88 +57:51:16.7
136.69708 -2.15127 galactic Cas Second-epoch detections are separated by 0.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx4120892 | 02:37:36.95 +57:51:15.9 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE J-Ks=0.719+/-0.036 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:36.88 +57:51:16.7: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:36.88 +57:51:16.7: 10.42 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.42 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 37 36.88 +57 51 16.7 7.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx4120892,2461199.8322,7.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx4120892 20260608.3322 7.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.80 02:33:01.74 +57:02:07.9
136.44839 -3.14612 galactic Per Second-epoch detections are separated by 0.4" and 8.4 pix
The object was found in VSX 4" GSC 03695-01369
Type: SR
# Max. Min./Amp. JD0 Period
9.750 R1 10.150 R1 2451481.00000 36.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:01.74 +57:02:07.9: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:01.74 +57:02:07.9: 10.93 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.93 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 01.74 +57 02 07.9 7.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GSC 03695-01369,2461199.8322,7.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 03695-01369 20260608.3322 7.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.83 02:19:52.93 +56:15:40.7
135.03717 -4.51758 galactic Per Second-epoch detections are separated by 0.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458262328911050880 | 02:19:52.94 +56:15:39.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.175+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:52.93 +56:15:40.7: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:52.93 +56:15:40.7: 10.47 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.47 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 19 52.93 +56 15 40.7 7.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458262328911050880,2461199.8322,7.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458262328911050880 20260608.3322 7.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.83 02:22:10.20 +56:24:23.3
135.28669 -4.27324 galactic Per Second-epoch detections are separated by 0.4" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx3989024 | 02:22:10.19 +56:24:23.4 (Gaia DR3) | (GCVS) | (GCVS) | Gaia3var=NOT_AVAILABLE J-Ks=0.108+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:10.20 +56:24:23.3: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:10.20 +56:24:23.3: 10.45 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.45 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 10.20 +56 24 23.3 7.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3989024,2461199.8322,7.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3989024 20260608.3322 7.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.84 02:19:48.61 +56:23:45.9
134.98233 -4.39399 galactic Per Second-epoch detections are separated by 0.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:19:48.61 +56:23:45.9 (user input) | T | P | (position from user input) J-Ks=0.372+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:48.61 +56:23:45.9: 13.20 +/- 0.36 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:48.61 +56:23:45.9: 10.51 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.51 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 19 48.61 +56 23 45.9 7.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,7.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 7.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.88 02:19:36.43 +56:14:20.7
135.00855 -4.55133 galactic Per Second-epoch detections are separated by 0.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J034.8921+56.2341 | 02:19:36.45 +56:14:19.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1959LS....C01....0H LS I +56 44 J-Ks=-0.055+/-0.032 (B)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:36.43 +56:14:20.7: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:36.43 +56:14:20.7: 10.53 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.53 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 19 36.43 +56 14 20.7 7.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J034.8921+56.2341,2461199.8322,7.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J034.8921+56.2341 20260608.3322 7.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.99 02:27:48.55 +57:05:55.3
135.76552 -3.35223 galactic Per Second-epoch detections are separated by 0.6" and 8.4 pix
The object was found in VSX 5" DP Per
Type: LB
# Max. Min./Amp. JD0 Period
14.200 pg 15.100 pg M6.5
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:48.55 +57:05:55.3: 10.21 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:48.55 +57:05:55.3: 11.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 48.55 +57 05 55.3 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DP Per,2461199.8322,7.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DP Per 20260608.3322 7.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.88 02:24:42.01 +56:55:47.8
135.43034 -3.66145 galactic Per Second-epoch detections are separated by 0.9" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.1620+56.9296 | 02:24:42.01 +56:55:47.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.133+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:42.01 +56:55:47.8: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:42.01 +56:55:47.8: 10.74 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.74 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 42.01 +56 55 47.8 7.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.1620+56.9296,2461199.8322,7.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.1620+56.9296 20260608.3322 7.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.88 02:32:45.26 +57:08:08.0
136.37560 -3.06791 galactic Per Second-epoch detections are separated by 1.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.1901+57.1255 | 02:32:45.21 +57:08:08.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.302+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:45.26 +57:08:08.0: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:45.26 +57:08:08.0: 10.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.52 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 45.26 +57 08 08.0 7.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.1901+57.1255,2461199.8322,7.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.1901+57.1255 20260608.3322 7.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.87 02:25:28.19 +56:11:20.2
135.79305 -4.31674 galactic Per Second-epoch detections are separated by 0.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457512943016360448 | 02:25:28.14 +56:11:20.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB- 1965LS....C05....0H LS V +55 6 J-Ks=-0.048+/-0.031 (B)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:28.19 +56:11:20.2: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:28.19 +56:11:20.2: 10.40 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.40 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 28.19 +56 11 20.2 7.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457512943016360448,2461199.8322,7.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457512943016360448 20260608.3322 7.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.92 02:25:20.40 +56:12:12.7
135.77092 -4.30953 galactic Per Second-epoch detections are separated by 1.0" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx4117142 | 02:25:20.28 +56:12:13.8 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE SpType: OB- 1965LS....C05....0H LS V +55 5 J-Ks=-0.059+/-0.034 (B)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:20.40 +56:12:12.7: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:20.40 +56:12:12.7: 10.44 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.44 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 20.40 +56 12 12.7 7.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx4117142,2461199.8322,7.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx4117142 20260608.3322 7.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.96 02:18:48.49 +56:17:54.8
134.88375 -4.53227 galactic Per Second-epoch detections are separated by 0.9" and 8.3 pix
The object was found in VSX11" Gaia DR3 458265180769332096
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.240 G 14.270 G 0.029804400000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:48.49 +56:17:54.8: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:48.49 +56:17:54.8: 10.56 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.56 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 18 48.49 +56 17 54.8 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458265180769332096,2461199.8322,7.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458265180769332096 20260608.3322 7.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.97 02:23:42.88 +56:07:10.8
135.58823 -4.46781 galactic Per Second-epoch detections are separated by 0.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx4123818 | 02:23:42.88 +56:07:10.8 (user input) | (GCVS) | (GCVS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:42.88 +56:07:10.8: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:42.88 +56:07:10.8: 10.63 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.63 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 42.88 +56 07 10.8 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx4123818,2461199.8322,7.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx4123818 20260608.3322 7.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.95 02:21:54.94 +56:42:38.7
135.14886 -3.99953 galactic Per Second-epoch detections are separated by 0.7" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx90481 | 02:21:54.86 +56:42:39.2 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE J-Ks=0.101+/-0.030 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:54.94 +56:42:38.7: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:54.94 +56:42:38.7: 10.53 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.53 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 54.94 +56 42 38.7 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx90481,2461199.8322,7.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx90481 20260608.3322 7.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.04 02:20:55.04 +56:23:19.2
135.12947 -4.34923 galactic Per Second-epoch detections are separated by 1.9" and 8.5 pix
The object was found in VSX 1" Gaia DR3 458269991132811904
Type: BE|GCAS|S
# Max. Min./Amp. JD0 Period
10.440 G 10.590 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:55.04 +56:23:19.2: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:55.04 +56:23:19.2: 10.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.70 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 20 55.04 +56 23 19.2 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458269991132811904,2461199.8322,8.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458269991132811904 20260608.3322 8.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.03 02:20:32.11 +56:10:00.6
135.15486 -4.57591 galactic Per Second-epoch detections are separated by 1.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458249512728852864 | 02:20:32.03 +56:09:58.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.234+/-0.036 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:32.11 +56:10:00.6: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:32.11 +56:10:00.6: 10.65 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.65 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 20 32.11 +56 10 00.6 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458249512728852864,2461199.8322,8.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458249512728852864 20260608.3322 8.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.98 02:27:07.72 +56:33:53.0
135.87274 -3.88359 galactic Per Second-epoch detections are separated by 1.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457618423109114880 | 02:27:07.78 +56:33:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.740+/-0.025 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:07.72 +56:33:53.0: 12.89 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:07.72 +56:33:53.0: 10.69 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.69 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 07.72 +56 33 53.0 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457618423109114880,2461199.8322,7.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457618423109114880 20260608.3322 7.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.04 02:23:57.26 +57:12:24.5
135.23774 -3.43790 galactic Per Second-epoch detections are separated by 4.2" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 458411484534727936 | 02:23:57.26 +57:12:22.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.334+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:57.26 +57:12:24.5: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:57.26 +57:12:24.5: 10.73 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.73 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 57.26 +57 12 24.5 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 458411484534727936,2461199.8322,8.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 458411484534727936 20260608.3322 8.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.00 02:31:12.06 +57:09:47.8
136.16984 -3.12200 galactic Per Second-epoch detections are separated by 1.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.7864+57.1721 | 02:31:12.06 +57:09:47.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.198+/-0.073 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:12.06 +57:09:47.8: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:12.06 +57:09:47.8: 10.78 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.78 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 12.06 +57 09 47.8 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.7864+57.1721,2461199.8322,8.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.7864+57.1721 20260608.3322 8.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.04 02:24:09.74 +56:34:02.3
135.48915 -4.02682 galactic Per Second-epoch detections are separated by 1.0" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:24:09.74 +56:34:02.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:09.74 +56:34:02.3: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:09.74 +56:34:02.3: 10.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.59 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 09.74 +56 34 02.3 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,8.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 8.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.06 02:22:04.60 +57:10:38.0
135.00903 -3.55388 galactic Per Second-epoch detections are separated by 1.4" and 8.2 pix
The object was found in VSX 1" NSV 800
Type: GCAS:
# Max. Min./Amp. JD0 Period
10.380 V Y 0.040 V B2Vn(e)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:04.60 +57:10:38.0: 11.38 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:04.60 +57:10:38.0: 10.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 04.60 +57 10 38.0 8.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 800,2461199.8322,8.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 800 20260608.3322 8.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.84 02:31:25.89 +56:07:05.1
136.59349 -4.07838 galactic Per Second-epoch detections are separated by 4.4" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457379661591549312 | 02:31:25.96 +56:07:00.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:25.89 +56:07:05.1: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:25.89 +56:07:05.1: 10.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.59 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 25.89 +56 07 05.1 7.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457379661591549312,2461199.8322,7.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457379661591549312 20260608.3322 7.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.92 02:32:04.83 +56:49:24.9
136.40935 -3.39136 galactic Per Second-epoch detections are separated by 1.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:32:04.83 +56:49:24.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:04.83 +56:49:24.9: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:04.83 +56:49:24.9: 10.36 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.36 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 04.83 +56 49 24.9 7.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,7.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 7.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.04 02:22:53.49 +56:47:13.1
135.24837 -3.88185 galactic Per Second-epoch detections are separated by 0.1" and 8.2 pix
The object was found in VSX22" Gaia DR3 458293905511244800
Type: E
# Max. Min./Amp. JD0 Period
17.130 G 17.440 G 7.070100000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:53.49 +56:47:13.1: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:53.49 +56:47:13.1: 10.63 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.63 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 53.49 +56 47 13.1 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458293905511244800,2461199.8322,8.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458293905511244800 20260608.3322 8.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.99 02:33:49.40 +57:35:12.5
136.33582 -2.59587 galactic Per Second-epoch detections are separated by 0.5" and 8.5 pix
The object was found in VSX19" ZTF J023348.90+573530.8
Type: BY
# Max. Min./Amp. JD0 Period
19.921 r Y 0.213 r 2458379.92900 0.792993600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:49.40 +57:35:12.5: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:49.40 +57:35:12.5: 10.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.54 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 49.40 +57 35 12.5 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J023348.90+573530.8,2461199.8322,7.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J023348.90+573530.8 20260608.3322 7.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.06 02:35:18.48 +57:31:39.8
136.54249 -2.57318 galactic Per Second-epoch detections are separated by 0.7" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458102246888080768 | 02:35:18.44 +57:31:40.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.222+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:18.48 +57:31:39.8: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:18.48 +57:31:39.8: 10.66 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.66 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 35 18.48 +57 31 39.8 8.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458102246888080768,2461199.8322,8.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458102246888080768 20260608.3322 8.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.01 02:30:51.91 +57:04:09.8
136.16281 -3.22613 galactic Per Second-epoch detections are separated by 0.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.7008+57.0647 | 02:30:51.91 +57:04:09.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:51.91 +57:04:09.8: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:51.91 +57:04:09.8: 10.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.54 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 51.91 +57 04 09.8 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.7008+57.0647,2461199.8322,8.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.7008+57.0647 20260608.3322 8.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.91 02:38:46.76 +57:49:57.1
136.84806 -2.10954 galactic Cas Second-epoch detections are separated by 0.6" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457946459832991616 | 02:38:46.61 +57:49:58.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1978A&AS...32...25R BD+57 603 J-Ks=0.250+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:46.76 +57:49:57.1: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:46.76 +57:49:57.1: 10.34 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.34 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 38 46.76 +57 49 57.1 7.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457946459832991616,2461199.8322,7.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457946459832991616 20260608.3322 7.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.03 02:25:33.89 +56:34:21.9
135.66834 -3.95341 galactic Per Second-epoch detections are separated by 1.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.4026+56.5763 | 02:25:33.89 +56:34:21.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:33.89 +56:34:21.9: 11.92 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:33.89 +56:34:21.9: 10.60 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.60 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 33.89 +56 34 21.9 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.4026+56.5763,2461199.8322,8.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.4026+56.5763 20260608.3322 8.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.21 02:30:00.34 +57:28:19.7
135.90438 -2.89582 galactic Per Second-epoch detections are separated by 1.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx181226 | 02:30:00.34 +57:28:19.7 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=1.283+/-0.036 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:00.34 +57:28:19.7: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:00.34 +57:28:19.7: 11.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 00.34 +57 28 19.7 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx181226,2461199.8322,8.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx181226 20260608.3322 8.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.97 02:28:50.69 +56:20:49.6
136.17357 -3.99971 galactic Per Second-epoch detections are separated by 1.6" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457554415218933120 | 02:28:50.80 +56:20:47.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.101+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:50.69 +56:20:49.6: 13.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:50.69 +56:20:49.6: 10.66 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.66 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 28 50.69 +56 20 49.6 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457554415218933120,2461199.8322,7.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457554415218933120 20260608.3322 7.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.10 02:31:38.55 +57:13:46.4
136.20031 -3.03808 galactic Per Second-epoch detections are separated by 0.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457989856183731328 | 02:31:38.47 +57:13:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.311+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:38.55 +57:13:46.4: 9.41 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:38.55 +57:13:46.4: 10.63 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.54 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 38.55 +57 13 46.4 8.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457989856183731328,2461199.8322,8.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457989856183731328 20260608.3322 8.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.12 02:36:35.03 +57:36:36.2
136.66765 -2.43035 galactic Cas Second-epoch detections are separated by 0.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457921720823408384 | 02:36:35.02 +57:36:36.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.303+/-0.027 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:35.03 +57:36:36.2: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:35.03 +57:36:36.2: 10.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.71 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 36 35.03 +57 36 36.2 8.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457921720823408384,2461199.8322,8.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457921720823408384 20260608.3322 8.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.19 02:24:06.49 +56:29:59.8
135.50585 -4.09252 galactic Per Second-epoch detections are separated by 1.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.0447+56.4918 | 02:24:06.53 +56:29:59.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.852+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:06.49 +56:29:59.8: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:06.49 +56:29:59.8: 10.90 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.90 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 06.49 +56 29 59.8 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.0447+56.4918,2461199.8322,8.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.0447+56.4918 20260608.3322 8.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.22 02:24:33.46 +56:57:18.3
135.40324 -3.64478 galactic Per Second-epoch detections are separated by 0.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx186151 | 02:24:33.44 +56:57:19.1 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE J-Ks=0.063+/-0.034 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:33.46 +56:57:18.3: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:33.46 +56:57:18.3: 10.81 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.81 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 33.46 +56 57 18.3 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx186151,2461199.8322,8.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx186151 20260608.3322 8.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.21 02:19:39.63 +56:20:11.8
134.98276 -4.45697 galactic Per Second-epoch detections are separated by 0.9" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J034.9014+56.3302 | 02:19:39.69 +56:20:10.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.622+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:39.63 +56:20:11.8: 9.87 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:39.63 +56:20:11.8: 10.94 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.88 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 19 39.63 +56 20 11.8 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J034.9014+56.3302,2461199.8322,8.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J034.9014+56.3302 20260608.3322 8.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.16 02:29:17.13 +57:14:30.0
135.89951 -3.14587 galactic Per Second-epoch detections are separated by 0.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458035554638504832 | 02:29:17.11 +57:14:29.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.781+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:17.13 +57:14:30.0: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:17.13 +57:14:30.0: 10.81 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.81 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 17.13 +57 14 30.0 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458035554638504832,2461199.8322,8.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458035554638504832 20260608.3322 8.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.23 02:26:07.35 +56:25:11.7
135.79512 -4.06867 galactic Per Second-epoch detections are separated by 0.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457610077996536576 | 02:26:07.34 +56:25:12.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.169+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:07.35 +56:25:11.7: 11.81 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:07.35 +56:25:11.7: 10.81 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.81 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 07.35 +56 25 11.7 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457610077996536576,2461199.8322,8.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457610077996536576 20260608.3322 8.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.22 02:21:55.92 +56:44:53.0
135.13814 -3.96372 galactic Per Second-epoch detections are separated by 0.3" and 8.2 pix
The object was found in VSX25" Gaia DR3 458304488310702848
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.850 G 13.880 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:55.92 +56:44:53.0: 13.15 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:55.92 +56:44:53.0: 10.83 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 55.92 +56 44 53.0 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458304488310702848,2461199.8322,8.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458304488310702848 20260608.3322 8.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.21 02:35:20.24 +57:29:29.9
136.56021 -2.60487 galactic Per Second-epoch detections are separated by 0.7" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.8552+57.4916 | 02:35:20.17 +57:29:30.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.125+/-0.029 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:20.24 +57:29:29.9: 13.04 +/- 0.31 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:20.24 +57:29:29.9: 10.86 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.86 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 35 20.24 +57 29 29.9 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.8552+57.4916,2461199.8322,8.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.8552+57.4916 20260608.3322 8.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.26 02:19:45.17 +56:31:44.3
134.93013 -4.27146 galactic Per Second-epoch detections are separated by 0.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458275626129683712 | 02:19:45.21 +56:31:46.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.630+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:45.17 +56:31:44.3: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:45.17 +56:31:44.3: 10.92 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.92 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 19 45.17 +56 31 44.3 8.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458275626129683712,2461199.8322,8.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458275626129683712 20260608.3322 8.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.29 02:21:04.75 +56:15:32.3
135.19486 -4.46357 galactic Per Second-epoch detections are separated by 1.7" and 8.3 pix
The object was found in VSX13" Gaia DR3 458255319524584576
Type: ROT
# Max. Min./Amp. JD0 Period
15.290 G 15.310 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:04.75 +56:15:32.3: 12.45 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:04.75 +56:15:32.3: 11.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.06 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 04.75 +56 15 32.3 8.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458255319524584576,2461199.8322,8.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458255319524584576 20260608.3322 8.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.23 02:30:33.01 +56:53:09.2
136.19172 -3.41236 galactic Per Second-epoch detections are separated by 1.0" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457978483110691456 | 02:30:32.95 +56:53:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.097+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:33.01 +56:53:09.2: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:33.01 +56:53:09.2: 10.78 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.78 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 33.01 +56 53 09.2 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457978483110691456,2461199.8322,8.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457978483110691456 20260608.3322 8.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.07 02:33:48.55 +57:01:45.9
136.54889 -3.11104 galactic Per Second-epoch detections are separated by 2.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.4387+57.0274 | 02:33:48.47 +57:01:46.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.306+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:48.55 +57:01:45.9: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:48.55 +57:01:45.9: 10.43 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.43 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 48.55 +57 01 45.9 8.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.4387+57.0274,2461199.8322,8.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.4387+57.0274 20260608.3322 8.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.16 02:31:18.70 +55:53:50.8
136.66132 -4.28906 galactic Per Second-epoch detections are separated by 5.3" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx532064 | 02:31:18.96 +55:53:50.0 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE J-Ks=0.878+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:18.70 +55:53:50.8: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:18.70 +55:53:50.8: 10.81 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.81 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 18.70 +55 53 50.8 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx532064,2461199.8322,8.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx532064 20260608.3322 8.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.25 02:36:08.52 +57:39:33.9
136.59380 -2.40825 galactic Cas Second-epoch detections are separated by 1.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.0481+57.6598 | 02:36:08.50 +57:39:34.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.314+/-0.027 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:08.52 +57:39:33.9: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:08.52 +57:39:33.9: 10.91 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.91 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 36 08.52 +57 39 33.9 8.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.0481+57.6598,2461199.8322,8.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.0481+57.6598 20260608.3322 8.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.23 02:30:32.25 +57:11:26.3
136.07608 -3.13032 galactic Per Second-epoch detections are separated by 1.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457986145332046080 | 02:30:32.15 +57:11:25.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.196+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:32.25 +57:11:26.3: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:32.25 +57:11:26.3: 10.80 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.80 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 32.25 +57 11 26.3 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457986145332046080,2461199.8322,8.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457986145332046080 20260608.3322 8.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.40 02:21:59.09 +56:30:01.6
135.23021 -4.19379 galactic Per Second-epoch detections are separated by 1.9" and 8.4 pix
The object was found in VSX 2" TYC 3694-1258-1
Type: SRS
# Max. Min./Amp. JD0 Period
11.810 V 12.020 V 2455719.00000 24.100000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:59.09 +56:30:01.6: 11.32 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:59.09 +56:30:01.6: 11.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 59.09 +56 30 01.6 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TYC 3694-1258-1,2461199.8322,8.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TYC 3694-1258-1 20260608.3322 8.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.37 02:25:03.15 +56:56:58.8
135.46840 -3.62601 galactic Per Second-epoch detections are separated by 2.6" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:25:03.15 +56:56:58.8 (user input) | T | P | (position from user input) J-Ks=0.947+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:03.15 +56:56:58.8: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:03.15 +56:56:58.8: 11.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.13 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 03.15 +56 56 58.8 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,8.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 8.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.30 02:22:31.56 +56:14:10.7
135.39200 -4.41595 galactic Per Second-epoch detections are separated by 0.6" and 8.2 pix
The object was found in VSX15" Gaia DR3 457502291496530304
Type: ROT
# Max. Min./Amp. JD0 Period
16.090 G 16.130 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:31.56 +56:14:10.7: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:31.56 +56:14:10.7: 10.87 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.87 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 31.56 +56 14 10.7 8.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457502291496530304,2461199.8322,8.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457502291496530304 20260608.3322 8.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.31 02:24:18.81 +56:54:02.0
135.39123 -3.70754 galactic Per Second-epoch detections are separated by 1.0" and 8.4 pix
The object was found in VSX19" Gaia DR3 458386298846823680
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
17.620 G 17.700 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:18.81 +56:54:02.0: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:18.81 +56:54:02.0: 10.94 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.94 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 18.81 +56 54 02.0 8.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458386298846823680,2461199.8322,8.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458386298846823680 20260608.3322 8.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.34 02:25:00.78 +56:51:31.9
135.49557 -3.71284 galactic Per Second-epoch detections are separated by 1.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 457640348919934208 | 02:25:00.75 +56:51:33.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.114+/-0.042 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:00.78 +56:51:31.9: 13.17 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:00.78 +56:51:31.9: 10.97 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.97 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 00.78 +56 51 31.9 8.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 457640348919934208,2461199.8322,8.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 457640348919934208 20260608.3322 8.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.37 02:19:56.52 +56:13:26.0
135.05764 -4.55003 galactic Per Second-epoch detections are separated by 1.4" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458261469917614080 | 02:19:56.64 +56:13:24.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5) J-Ks=0.056+/-0.041 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:56.52 +56:13:26.0: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:56.52 +56:13:26.0: 11.04 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.04 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 19 56.52 +56 13 26.0 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458261469917614080,2461199.8322,8.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458261469917614080 20260608.3322 8.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.28 02:26:13.46 +56:36:46.9
135.73890 -3.88335 galactic Per Second-epoch detections are separated by 1.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:26:13.46 +56:36:46.9 (user input) | T | P | (position from user input) J-Ks=0.082+/-0.029 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:13.46 +56:36:46.9: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:13.46 +56:36:46.9: 10.79 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.79 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 13.46 +56 36 46.9 8.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,8.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 8.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.18 02:27:33.11 +56:13:09.8
136.05296 -4.18420 galactic Per Second-epoch detections are separated by 2.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457557060918681856 | 02:27:33.13 +56:13:10.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.062+/-0.026 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:33.11 +56:13:09.8: 11.32 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:33.11 +56:13:09.8: 10.64 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.64 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 33.11 +56 13 09.8 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457557060918681856,2461199.8322,8.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457557060918681856 20260608.3322 8.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.37 02:29:26.34 +57:23:02.8
135.86611 -3.00584 galactic Per Second-epoch detections are separated by 0.5" and 8.4 pix
The object was found in VSX 1" Gaia DR3 458044728688621568
Type: E
# Max. Min./Amp. JD0 Period
10.720 G 10.820 G 0.776180000000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:26.34 +57:23:02.8: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:26.34 +57:23:02.8: 11.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 26.34 +57 23 02.8 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458044728688621568,2461199.8322,8.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458044728688621568 20260608.3322 8.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.42 02:23:02.19 +56:30:28.6
135.36414 -4.13664 galactic Per Second-epoch detections are separated by 2.0" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:23:02.19 +56:30:28.6 (user input) | T | P | (position from user input) SpType: B 1965LS....C05....0H LS V +56 40 J-Ks=-0.038+/-0.034 (B)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:02.19 +56:30:28.6: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:02.19 +56:30:28.6: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 02.19 +56 30 28.6 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,8.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 8.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.37 02:31:20.24 +57:33:46.4
136.03643 -2.74481 galactic Per Second-epoch detections are separated by 1.0" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458067234316909312 | 02:31:20.25 +57:33:46.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.337+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:20.24 +57:33:46.4: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:20.24 +57:33:46.4: 10.97 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.97 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 20.24 +57 33 46.4 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458067234316909312,2461199.8322,8.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458067234316909312 20260608.3322 8.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.42 02:24:32.63 +57:00:44.1
135.38129 -3.59194 galactic Per Second-epoch detections are separated by 0.5" and 8.3 pix
The object was found in VSX 1" Barlad V48
Type:
# Max. Min./Amp. JD0 Period
10.990 V Y 0.280 TESS 2457271.73600 0.662760000000 B3e
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:32.63 +57:00:44.1: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:32.63 +57:00:44.1: 10.97 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.97 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 32.63 +57 00 44.1 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Barlad V48,2461199.8322,8.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Barlad V48 20260608.3322 8.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.38 02:29:28.55 +56:33:06.0
136.17915 -3.77742 galactic Per Second-epoch detections are separated by 1.6" and 8.1 pix
The object was found in VSX 1" Gaia DR3 457591145780012800
Type: BCEP
# Max. Min./Amp. JD0 Period
10.740 G 10.780 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:28.55 +56:33:06.0: 13.08 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:28.55 +56:33:06.0: 10.93 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.93 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 28.55 +56 33 06.0 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457591145780012800,2461199.8322,8.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457591145780012800 20260608.3322 8.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.49 02:16:52.43 +56:18:43.8
134.62509 -4.60760 galactic Per Second-epoch detections are separated by 1.1" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J034.2189+56.3127 | 02:16:52.43 +56:18:43.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.251+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:52.43 +56:18:43.8: 11.81 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:52.43 +56:18:43.8: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 16 52.43 +56 18 43.8 8.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J034.2189+56.3127,2461199.8322,8.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J034.2189+56.3127 20260608.3322 8.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.47 02:18:24.03 +56:23:21.4
134.80014 -4.46540 galactic Per Second-epoch detections are separated by 0.9" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx590719 | 02:18:24.08 +56:23:24.9 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:24.03 +56:23:21.4: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:24.03 +56:23:21.4: 11.09 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.09 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 18 24.03 +56 23 21.4 8.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx590719,2461199.8322,8.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx590719 20260608.3322 8.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.43 02:26:55.75 +56:30:20.2
135.86845 -3.94864 galactic Per Second-epoch detections are separated by 0.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457617843297470592 | 02:26:55.70 +56:30:20.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.099+/-0.028 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:55.75 +56:30:20.2: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:55.75 +56:30:20.2: 11.05 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.05 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 55.75 +56 30 20.2 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457617843297470592,2461199.8322,8.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457617843297470592 20260608.3322 8.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.51 02:30:30.83 +57:30:27.8
135.95455 -2.83737 galactic Per Second-epoch detections are separated by 2.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458046515393935744 | 02:30:30.94 +57:30:26.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.350+/-0.035 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:30.83 +57:30:27.8: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:30.83 +57:30:27.8: 11.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.50 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 30.83 +57 30 27.8 8.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458046515393935744,2461199.8322,8.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458046515393935744 20260608.3322 8.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.48 02:23:48.03 +56:47:01.5
135.36645 -3.84153 galactic Per Second-epoch detections are separated by 0.1" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:23:48.03 +56:47:01.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:48.03 +56:47:01.5: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:48.03 +56:47:01.5: 11.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.06 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 48.03 +56 47 01.5 8.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,8.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 8.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.48 02:26:10.79 +56:48:28.8
135.66315 -3.70352 galactic Per Second-epoch detections are separated by 0.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457637668866212864 | 02:26:10.73 +56:48:29.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.384+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:10.79 +56:48:28.8: 10.57 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:10.79 +56:48:28.8: 11.09 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.08 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 10.79 +56 48 28.8 8.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457637668866212864,2461199.8322,8.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457637668866212864 20260608.3322 8.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.42 02:33:09.10 +57:00:38.5
136.47335 -3.16268 galactic Per Second-epoch detections are separated by 1.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.2979+57.0026 | 02:33:09.28 +57:00:39.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.196+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:09.10 +57:00:38.5: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:09.10 +57:00:38.5: 10.97 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.97 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 09.10 +57 00 38.5 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.2979+57.0026,2461199.8322,8.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.2979+57.0026 20260608.3322 8.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.53 02:33:40.71 +57:26:09.7
136.37592 -2.74253 galactic Per Second-epoch detections are separated by 1.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 458009784833002752 | 02:33:40.74 +57:26:10.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: B 1965LS....C05....0H LS V +57 51 J-Ks=0.185+/-0.028 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:40.71 +57:26:09.7: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:40.71 +57:26:09.7: 11.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.13 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 40.71 +57 26 09.7 8.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 458009784833002752,2461199.8322,8.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 458009784833002752 20260608.3322 8.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.46 02:36:22.58 +57:40:05.6
136.61916 -2.38783 galactic Cas Second-epoch detections are separated by 0.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458109771665185536 | 02:36:22.54 +57:40:06.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.267+/-0.047 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:22.58 +57:40:05.6: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:22.58 +57:40:05.6: 11.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.06 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 36 22.58 +57 40 05.6 8.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458109771665185536,2461199.8322,8.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458109771665185536 20260608.3322 8.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.55 02:25:48.44 +56:55:12.4
135.57535 -3.61702 galactic Per Second-epoch detections are separated by 1.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457641826394416640 | 02:25:48.39 +56:55:12.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.079+/-0.029 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:48.44 +56:55:12.4: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:48.44 +56:55:12.4: 11.14 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.14 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 48.44 +56 55 12.4 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457641826394416640,2461199.8322,8.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457641826394416640 20260608.3322 8.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.58 02:23:17.91 +56:42:23.9
135.32878 -3.93781 galactic Per Second-epoch detections are separated by 0.7" and 8.3 pix
The object was found in VSX 1" Gaia DR3 458289473105316864
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.020 G 11.050 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:17.91 +56:42:23.9: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:17.91 +56:42:23.9: 11.16 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.16 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 17.91 +56 42 23.9 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458289473105316864,2461199.8322,8.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458289473105316864 20260608.3322 8.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.64 02:20:18.71 +56:31:49.5
135.00242 -4.24417 galactic Per Second-epoch detections are separated by 2.3" and 8.5 pix
The object was found in VSX17" ZTF J022018.55+563206.7
Type: SR
# Max. Min./Amp. JD0 Period
14.253 r Y 0.230 r 2458375.81050 70.681770000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:18.71 +56:31:49.5: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:18.71 +56:31:49.5: 11.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 20 18.71 +56 31 49.5 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J022018.55+563206.7,2461199.8322,8.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J022018.55+563206.7 20260608.3322 8.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.60 02:21:34.57 +56:26:43.9
135.19593 -4.26472 galactic Per Second-epoch detections are separated by 2.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.4115+56.4466 | 02:21:34.45 +56:26:43.9 (Gaia DR3) | LPV (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.038+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:34.57 +56:26:43.9: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:34.57 +56:26:43.9: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 34.57 +56 26 43.9 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.4115+56.4466,2461199.8322,8.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.4115+56.4466 20260608.3322 8.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.62 02:19:36.20 +56:23:21.9
134.95753 -4.40987 galactic Per Second-epoch detections are separated by 1.4" and 8.3 pix
The object was found in VSX 4" Gaia DR3 458272396314337536
Type: S
# Max. Min./Amp. JD0 Period
15.810 G 16.200 G M
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:36.20 +56:23:21.9: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:36.20 +56:23:21.9: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 19 36.20 +56 23 21.9 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458272396314337536,2461199.8322,8.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458272396314337536 20260608.3322 8.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.62 02:25:56.01 +56:58:59.2
135.56890 -3.55204 galactic Per Second-epoch detections are separated by 1.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.4932+56.9802 | 02:25:56.01 +56:58:59.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.464+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:56.01 +56:58:59.2: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:56.01 +56:58:59.2: 11.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.23 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 56.01 +56 58 59.2 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.4932+56.9802,2461199.8322,8.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.4932+56.9802 20260608.3322 8.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.61 02:35:08.67 +57:36:14.5
136.49251 -2.51146 galactic Cas Second-epoch detections are separated by 0.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458105717221633536 | 02:35:08.75 +57:36:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.847+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:08.67 +57:36:14.5: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:08.67 +57:36:14.5: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 35 08.67 +57 36 14.5 8.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458105717221633536,2461199.8322,8.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458105717221633536 20260608.3322 8.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.57 02:37:50.64 +57:45:49.7
136.76133 -2.22241 galactic Cas Second-epoch detections are separated by 0.9" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.4571+57.7717 | 02:37:50.64 +57:45:49.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: OB- 1959LS....C01....0H LS I +57 75
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:50.64 +57:45:49.7: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:50.64 +57:45:49.7: 11.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 37 50.64 +57 45 49.7 8.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.4571+57.7717,2461199.8322,8.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.4571+57.7717 20260608.3322 8.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.54 02:26:43.23 +56:24:12.4
135.87844 -4.05433 galactic Per Second-epoch detections are separated by 1.1" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.6811+56.4136 | 02:26:43.23 +56:24:12.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:43.23 +56:24:12.4: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:43.23 +56:24:12.4: 11.12 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.12 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 43.23 +56 24 12.4 8.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.6811+56.4136,2461199.8322,8.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.6811+56.4136 20260608.3322 8.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.64 02:35:04.64 +57:26:52.9
136.54500 -2.65866 galactic Per Second-epoch detections are separated by 1.1" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458007791968161280 | 02:35:04.80 +57:26:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.761+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:04.64 +57:26:52.9: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:04.64 +57:26:52.9: 11.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 35 04.64 +57 26 52.9 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458007791968161280,2461199.8322,8.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458007791968161280 20260608.3322 8.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.65 02:24:34.14 +56:53:00.2
135.43001 -3.71133 galactic Per Second-epoch detections are separated by 1.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458391177929671040 | 02:24:34.08 +56:53:01.2 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.213+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:34.14 +56:53:00.2: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:34.14 +56:53:00.2: 11.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.32 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 34.14 +56 53 00.2 8.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458391177929671040,2461199.8322,8.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458391177929671040 20260608.3322 8.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.71 02:22:27.95 +56:41:51.9
135.22441 -3.98575 galactic Per Second-epoch detections are separated by 0.5" and 8.2 pix
The object was found in VSX24" Gaia DR3 458291706488051840
Type: ROT
# Max. Min./Amp. JD0 Period
16.080 G 16.120 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:27.95 +56:41:51.9: 12.89 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:27.95 +56:41:51.9: 11.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.28 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 27.95 +56 41 51.9 8.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458291706488051840,2461199.8322,8.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458291706488051840 20260608.3322 8.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.62 02:26:11.70 +56:56:03.6
135.61974 -3.58483 galactic Per Second-epoch detections are separated by 1.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 457665122298060800 | 02:26:11.60 +56:56:03.5 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.042+/-0.034 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:11.70 +56:56:03.6: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:11.70 +56:56:03.6: 11.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 11.70 +56 56 03.6 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 457665122298060800,2461199.8322,8.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 457665122298060800 20260608.3322 8.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.71 02:18:05.24 +56:15:07.5
134.80446 -4.60923 galactic Per Second-epoch detections are separated by 0.8" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 456810595604427392 | 02:18:01.38 +56:15:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 2013AJ....145..102L PM J02180+5616
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:05.24 +56:15:07.5: 12.05 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:05.24 +56:15:07.5: 11.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 18 05.24 +56 15 07.5 8.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 456810595604427392,2461199.8322,8.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 456810595604427392 20260608.3322 8.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.65 02:34:48.66 +57:38:04.9
136.43939 -2.50057 galactic Per Second-epoch detections are separated by 0.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.7029+57.6276 | 02:34:48.60 +57:38:04.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1959LS....C01....0H LS I +57 70
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:48.66 +57:38:04.9: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:48.66 +57:38:04.9: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 48.66 +57 38 04.9 8.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.7029+57.6276,2461199.8322,8.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.7029+57.6276 20260608.3322 8.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.62 02:27:59.53 +56:29:42.2
136.00928 -3.90524 galactic Per Second-epoch detections are separated by 2.2" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:27:59.53 +56:29:42.2 (user input) | T | P | (position from user input) J-Ks=0.153+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:59.53 +56:29:42.2: 13.06 +/- 0.31 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:59.53 +56:29:42.2: 11.15 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 59.53 +56 29 42.2 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,8.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 8.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.45 02:29:33.00 +55:57:16.1
136.41042 -4.32836 galactic Per Second-epoch detections are separated by 3.1" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457351177367649536 | 02:29:33.62 +55:57:17.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:33.00 +55:57:16.1: 13.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:33.00 +55:57:16.1: 11.03 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.03 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 33.00 +55 57 16.1 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457351177367649536,2461199.8322,8.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457351177367649536 20260608.3322 8.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.71 02:24:02.04 +56:49:22.3
135.38273 -3.79370 galactic Per Second-epoch detections are separated by 1.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458385405493688832 | 02:24:01.94 +56:49:22.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1965LS....C05....0H LS V +56 41 J-Ks=0.057+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:02.04 +56:49:22.3: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:02.04 +56:49:22.3: 11.27 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 02.04 +56 49 22.3 8.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458385405493688832,2461199.8322,8.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458385405493688832 20260608.3322 8.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.77 02:23:55.73 +56:44:45.5
135.39622 -3.87076 galactic Per Second-epoch detections are separated by 2.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.9890+56.7447 | 02:23:55.57 +56:44:45.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.057+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:55.73 +56:44:45.5: 12.14 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:55.73 +56:44:45.5: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 55.73 +56 44 45.5 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.9890+56.7447,2461199.8322,8.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.9890+56.7447 20260608.3322 8.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.79 02:21:52.12 +56:41:17.7
135.15053 -4.02288 galactic Per Second-epoch detections are separated by 0.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458303148280950272 | 02:21:52.08 +56:41:18.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.007+/-0.035 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:52.12 +56:41:17.7: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:52.12 +56:41:17.7: 11.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 52.12 +56 41 17.7 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458303148280950272,2461199.8322,8.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458303148280950272 20260608.3322 8.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.63 02:32:17.85 +57:17:09.3
136.26104 -2.95239 galactic Per Second-epoch detections are separated by 0.9" and 8.6 pix
The object was found in VSX 0" Gaia DR3 458013701843090176
Type: E
# Max. Min./Amp. JD0 Period
10.980 G 11.070 G 3.240760000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:17.85 +57:17:09.3: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:17.85 +57:17:09.3: 11.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.23 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 17.85 +57 17 09.3 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458013701843090176,2461199.8322,8.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458013701843090176 20260608.3322 8.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.79 02:23:38.21 +56:39:53.8
135.38700 -3.96069 galactic Per Second-epoch detections are separated by 0.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458288476672646272 | 02:23:38.16 +56:39:54.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.043+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:38.21 +56:39:53.8: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:38.21 +56:39:53.8: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 38.21 +56 39 53.8 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458288476672646272,2461199.8322,8.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458288476672646272 20260608.3322 8.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.64 02:31:29.32 +57:11:54.7
136.19272 -3.07467 galactic Per Second-epoch detections are separated by 0.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457988344355269888 | 02:31:29.21 +57:11:55.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.352+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:29.32 +57:11:54.7: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:29.32 +57:11:54.7: 11.18 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.18 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 29.32 +57 11 54.7 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457988344355269888,2461199.8322,8.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457988344355269888 20260608.3322 8.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.74 02:37:50.68 +57:57:56.9
136.68080 -2.03713 galactic Cas Second-epoch detections are separated by 0.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458138766987060992 | 02:37:50.73 +57:57:57.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.147+/-0.027 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:50.68 +57:57:56.9: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:50.68 +57:57:56.9: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 37 50.68 +57 57 56.9 8.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458138766987060992,2461199.8322,8.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458138766987060992 20260608.3322 8.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.93 02:21:30.49 +57:12:34.5
134.92543 -3.54985 galactic Per Second-epoch detections are separated by 4.9" and 9.0 pix
The object was found in VSX 5" Gaia DR3 458455980397964160
Type: RS
# Max. Min./Amp. JD0 Period
17.500 G 17.640 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:30.49 +57:12:34.5: 9.70 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:30.49 +57:12:34.5: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 30.49 +57 12 34.5 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458455980397964160,2461199.8322,8.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458455980397964160 20260608.3322 8.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.79 02:25:30.12 +56:16:52.8
135.76425 -4.22881 galactic Per Second-epoch detections are separated by 3.0" and 8.7 pix
The object was found in VSX16" Gaia DR3 457517925178383616
Type: E
# Max. Min./Amp. JD0 Period
16.000 G 16.110 G 1.956010000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:30.12 +56:16:52.8: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:30.12 +56:16:52.8: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 30.12 +56 16 52.8 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457517925178383616,2461199.8322,8.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457517925178383616 20260608.3322 8.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.65 02:31:09.75 +57:16:14.4
136.12459 -3.02444 galactic Per Second-epoch detections are separated by 1.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457993944995787520 | 02:31:09.65 +57:16:15.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.133+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:09.75 +57:16:14.4: 12.86 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:09.75 +57:16:14.4: 11.10 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.10 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 09.75 +57 16 14.4 8.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457993944995787520,2461199.8322,8.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457993944995787520 20260608.3322 8.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.84 02:20:07.36 +56:27:52.1
135.00007 -4.31506 galactic Per Second-epoch detections are separated by 1.4" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458274320459648000 | 02:20:07.35 +56:27:51.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.713+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:07.36 +56:27:52.1: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:07.36 +56:27:52.1: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 20 07.36 +56 27 52.1 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458274320459648000,2461199.8322,8.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458274320459648000 20260608.3322 8.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.85 02:33:34.12 +55:49:25.9
136.98303 -4.23655 galactic Per Second-epoch detections are separated by 8.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.3792+55.8236 | 02:33:34.38 +55:49:28.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:34.12 +55:49:25.9: 12.38 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:34.12 +55:49:25.9: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 34.12 +55 49 25.9 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.3792+55.8236,2461199.8322,8.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.3792+55.8236 20260608.3322 8.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.76 02:33:03.26 +57:03:29.0
136.44295 -3.12398 galactic Per Second-epoch detections are separated by 0.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.2584+57.0472 | 02:33:03.33 +57:03:28.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.027+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:03.26 +57:03:29.0: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:03.26 +57:03:29.0: 11.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.48 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 03.26 +57 03 29.0 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.2584+57.0472,2461199.8322,8.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.2584+57.0472 20260608.3322 8.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.78 02:33:10.59 +57:32:53.7
136.27047 -2.66476 galactic Per Second-epoch detections are separated by 1.3" and 8.6 pix
The object was found in ASASSN-V 0" ASASSN-V J023310.55+573254.1
Type: VAR
MeanMag 11.23 m Amp. 1.35 m Period 514.391279 d
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:10.59 +57:32:53.7: 12.71 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:10.59 +57:32:53.7: 11.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 10.59 +57 32 53.7 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461199.8322,8.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260608.3322 8.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.80 02:36:59.45 +57:56:29.8
136.58641 -2.10434 galactic Cas Second-epoch detections are separated by 4.1" and 9.2 pix
The object was found in VSX21" Gaia DR3 458140695435098880
Type: ROT
# Max. Min./Amp. JD0 Period
15.900 G 15.940 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:59.45 +57:56:29.8: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:59.45 +57:56:29.8: 11.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.48 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 36 59.45 +57 56 29.8 8.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458140695435098880,2461199.8322,8.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458140695435098880 20260608.3322 8.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.70 02:32:14.18 +55:56:22.8
136.76554 -4.20097 galactic Per Second-epoch detections are separated by 5.3" and 8.3 pix
The object was found in VSX 4" V1071 Per
Type: EW
# Max. Min./Amp. JD0 Period
10.940 V 11.240 V 2457070.72700 0.359847600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:14.18 +55:56:22.8: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:14.18 +55:56:22.8: 11.08 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.08 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 14.18 +55 56 22.8 8.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1071 Per,2461199.8322,8.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1071 Per 20260608.3322 8.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.82 02:25:56.75 +56:07:50.5
135.87598 -4.34751 galactic Per Second-epoch detections are separated by 0.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457464942460413568 | 02:25:56.69 +56:07:50.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.324+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:56.75 +56:07:50.5: 13.14 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:56.75 +56:07:50.5: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 56.75 +56 07 50.5 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457464942460413568,2461199.8322,8.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457464942460413568 20260608.3322 8.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.86 02:25:04.29 +56:13:07.5
135.73050 -4.30856 galactic Per Second-epoch detections are separated by 1.7" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457515824930594816 | 02:25:04.36 +56:13:09.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.337+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:04.29 +56:13:07.5: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:04.29 +56:13:07.5: 11.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 04.29 +56 13 07.5 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457515824930594816,2461199.8322,8.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457515824930594816 20260608.3322 8.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.59 02:33:34.41 +56:11:48.0
136.83992 -3.89216 galactic Per Second-epoch detections are separated by 4.5" and 8.4 pix
The object was found in VSX 6" Gaia DR3 457371518333663744
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.980 G 11.010 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:34.41 +56:11:48.0: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:34.41 +56:11:48.0: 11.03 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.03 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 34.41 +56 11 48.0 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457371518333663744,2461199.8322,8.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457371518333663744 20260608.3322 8.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.77 02:34:24.39 +57:28:26.1
136.45172 -2.66981 galactic Per Second-epoch detections are separated by 0.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.5831+57.4740 | 02:34:24.42 +57:28:26.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.152+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:24.39 +57:28:26.1: 10.05 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:24.39 +57:28:26.1: 11.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 24.39 +57 28 26.1 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.5831+57.4740,2461199.8322,8.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.5831+57.4740 20260608.3322 8.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.80 02:38:13.42 +57:50:16.2
136.77814 -2.13434 galactic Cas Second-epoch detections are separated by 0.8" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.5732+57.8385 | 02:38:13.32 +57:50:17.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.231+/-0.026 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:13.42 +57:50:16.2: 13.20 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:13.42 +57:50:16.2: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 38 13.42 +57 50 16.2 8.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.5732+57.8385,2461199.8322,8.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.5732+57.8385 20260608.3322 8.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.81 02:28:48.05 +56:30:07.8
136.11075 -3.85776 galactic Per Second-epoch detections are separated by 1.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457567987315527296 | 02:28:48.02 +56:30:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.190+/-0.040 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:48.05 +56:30:07.8: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:48.05 +56:30:07.8: 11.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 28 48.05 +56 30 07.8 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457567987315527296,2461199.8322,8.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457567987315527296 20260608.3322 8.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.81 02:33:54.63 +57:40:55.2
136.30991 -2.50352 galactic Per Second-epoch detections are separated by 0.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458119529835993600 | 02:33:54.62 +57:40:56.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB- 1965LS....C05....0H LS V +57 52 J-Ks=0.134+/-0.028 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:54.63 +57:40:55.2: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:54.63 +57:40:55.2: 11.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 54.63 +57 40 55.2 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458119529835993600,2461199.8322,8.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458119529835993600 20260608.3322 8.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.96 02:25:42.31 +56:37:12.9
135.66946 -3.90215 galactic Per Second-epoch detections are separated by 0.6" and 8.4 pix
The object was found in VSX 1" ASASSN-V J022542.34+563711.6
Type: SR
# Max. Min./Amp. JD0 Period
12.400 V 12.550 V 2458546.70420 284.180457300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:42.31 +56:37:12.9: 12.68 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:42.31 +56:37:12.9: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 42.31 +56 37 12.9 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J022542.34+563711.6,2461199.8322,8.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J022542.34+563711.6 20260608.3322 8.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.94 02:21:55.06 +56:20:50.1
135.27421 -4.34086 galactic Per Second-epoch detections are separated by 0.9" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458277893873461120 | 02:21:55.07 +56:20:50.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.360+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:55.06 +56:20:50.1: 8.69 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:55.06 +56:20:50.1: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.17 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 55.06 +56 20 50.1 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458277893873461120,2461199.8322,8.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458277893873461120 20260608.3322 8.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.97 02:24:25.89 +56:32:55.3
135.53052 -4.03120 galactic Per Second-epoch detections are separated by 1.3" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.1043+56.5466 | 02:24:25.88 +56:32:56.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.365+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:25.89 +56:32:55.3: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:25.89 +56:32:55.3: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 25.89 +56 32 55.3 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.1043+56.5466,2461199.8322,8.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.1043+56.5466 20260608.3322 8.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.95 02:24:47.99 +56:36:57.6
135.55428 -3.95033 galactic Per Second-epoch detections are separated by 0.1" and 8.3 pix
The object was found in VSX 2" Gaia DR3 457630522034972416
Type: ROT
# Max. Min./Amp. JD0 Period
11.410 G 11.460 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:47.99 +56:36:57.6: 12.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:47.99 +56:36:57.6: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 47.99 +56 36 57.6 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457630522034972416,2461199.8322,8.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457630522034972416 20260608.3322 8.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.95 02:24:32.13 +56:43:35.2
135.48116 -3.85981 galactic Per Second-epoch detections are separated by 2.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457633511337779584 | 02:24:32.08 +56:43:34.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.763+/-0.036 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:32.13 +56:43:35.2: 11.82 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:32.13 +56:43:35.2: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 32.13 +56 43 35.2 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457633511337779584,2461199.8322,8.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457633511337779584 20260608.3322 8.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.91 02:26:15.82 +56:04:34.0
135.93708 -4.38259 galactic Per Second-epoch detections are separated by 1.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457463774229697408 | 02:26:15.80 +56:04:32.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.817+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:15.82 +56:04:34.0: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:15.82 +56:04:34.0: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 15.82 +56 04 34.0 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457463774229697408,2461199.8322,8.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457463774229697408 20260608.3322 8.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.88 02:25:45.49 +56:26:32.2
135.73996 -4.06580 galactic Per Second-epoch detections are separated by 2.0" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457613239092461312 | 02:25:45.40 +56:26:32.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.083+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:45.49 +56:26:32.2: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:45.49 +56:26:32.2: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 45.49 +56 26 32.2 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457613239092461312,2461199.8322,8.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457613239092461312 20260608.3322 8.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.05 02:21:36.86 +56:40:52.1
135.12008 -4.04152 galactic Per Second-epoch detections are separated by 2.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458298063039684480 | 02:21:36.88 +56:40:52.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.860+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:36.86 +56:40:52.1: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:36.86 +56:40:52.1: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 36.86 +56 40 52.1 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458298063039684480,2461199.8322,9.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458298063039684480 20260608.3322 9.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.90 02:30:39.48 +57:13:42.2
136.07711 -3.08921 galactic Per Second-epoch detections are separated by 1.7" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 457992158286713856 | 02:30:39.37 +57:13:42.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.224+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:39.48 +57:13:42.2: 12.70 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:39.48 +57:13:42.2: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 39.48 +57 13 42.2 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 457992158286713856,2461199.8322,8.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 457992158286713856 20260608.3322 8.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.97 02:25:07.44 +56:14:04.5
135.73171 -4.29117 galactic Per Second-epoch detections are separated by 0.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457516207191491200 | 02:25:07.40 +56:14:05.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.001+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:07.44 +56:14:04.5: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:07.44 +56:14:04.5: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 07.44 +56 14 04.5 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457516207191491200,2461199.8322,8.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457516207191491200 20260608.3322 8.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.94 02:26:00.84 +56:46:18.0
135.65494 -3.74557 galactic Per Second-epoch detections are separated by 0.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457636122678005120 | 02:26:00.79 +56:46:18.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.239+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:00.84 +56:46:18.0: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:00.84 +56:46:18.0: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 00.84 +56 46 18.0 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457636122678005120,2461199.8322,8.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457636122678005120 20260608.3322 8.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.09 02:26:59.49 +57:14:44.2
135.60873 -3.25547 galactic Per Second-epoch detections are separated by 0.6" and 8.3 pix
The object was found in VSX 1" ASASSN-V J022659.55+571443.3
Type: SR
# Max. Min./Amp. JD0 Period
13.400 g Y 0.150 g 2458680.08400 226.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:59.49 +57:14:44.2: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:59.49 +57:14:44.2: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 59.49 +57 14 44.2 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J022659.55+571443.3,2461199.8322,9.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J022659.55+571443.3 20260608.3322 9.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.96 02:31:10.54 +57:30:46.6
136.03510 -2.79924 galactic Per Second-epoch detections are separated by 1.6" and 8.7 pix
The object was found in VSX11" Gaia DR3 458067062518240768
Type: RS
# Max. Min./Amp. JD0 Period
16.780 G 16.930 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:10.54 +57:30:46.6: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:10.54 +57:30:46.6: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 10.54 +57 30 46.6 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458067062518240768,2461199.8322,8.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458067062518240768 20260608.3322 8.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.91 02:29:57.33 +56:36:50.4
136.21745 -3.69504 galactic Per Second-epoch detections are separated by 3.1" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457581490693447040 | 02:29:57.38 +56:36:48.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.969+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:57.33 +56:36:50.4: 10.49 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:57.33 +56:36:50.4: 11.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 57.33 +56 36 50.4 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457581490693447040,2461199.8322,8.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457581490693447040 20260608.3322 8.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.94 02:31:12.57 +57:00:49.3
136.22722 -3.26018 galactic Per Second-epoch detections are separated by 1.0" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457980098018246784 | 02:31:12.49 +57:00:49.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.263+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:12.57 +57:00:49.3: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:12.57 +57:00:49.3: 11.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 12.57 +57 00 49.3 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457980098018246784,2461199.8322,8.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457980098018246784 20260608.3322 8.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.10 02:20:24.56 +56:41:43.6
134.95922 -4.08430 galactic Per Second-epoch detections are separated by 1.5" and 8.3 pix
The object was found in VSX 1" ASASSN-V J022024.69+564144.6
Type: L
# Max. Min./Amp. JD0 Period
12.350 V 12.450 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:24.56 +56:41:43.6: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:24.56 +56:41:43.6: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 20 24.56 +56 41 43.6 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J022024.69+564144.6,2461199.8322,9.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J022024.69+564144.6 20260608.3322 9.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.09 02:23:44.10 +56:55:56.9
135.30593 -3.70533 galactic Per Second-epoch detections are separated by 0.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 458390250206940928 | 02:23:44.07 +56:55:57.5 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.162+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:44.10 +56:55:56.9: 12.06 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:44.10 +56:55:56.9: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 44.10 +56 55 56.9 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 458390250206940928,2461199.8322,9.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 458390250206940928 20260608.3322 9.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.01 02:23:14.27 +56:52:06.4
135.26455 -3.78900 galactic Per Second-epoch detections are separated by 1.3" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.7911+56.8666 | 02:23:14.22 +56:52:07.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.051+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:14.27 +56:52:06.4: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:14.27 +56:52:06.4: 11.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 14.27 +56 52 06.4 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.7911+56.8666,2461199.8322,9.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.7911+56.8666 20260608.3322 9.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.97 02:26:08.97 +56:16:06.3
135.85305 -4.20877 galactic Per Second-epoch detections are separated by 1.0" and 8.5 pix
The object was found in VSX22" ZTF J022611.58+561604.9
Type: RS
# Max. Min./Amp. JD0 Period
19.739 r Y 0.357 r 2458514.61170 3.605615400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:08.97 +56:16:06.3: 10.64 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:08.97 +56:16:06.3: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 08.97 +56 16 06.3 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J022611.58+561604.9,2461199.8322,8.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J022611.58+561604.9 20260608.3322 8.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.99 02:33:43.78 +57:36:02.2
136.31891 -2.58796 galactic Per Second-epoch detections are separated by 2.3" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458025212355181952 | 02:33:43.70 +57:36:02.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2V (LAMOST DR5) J-Ks=0.139+/-0.028 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:43.78 +57:36:02.2: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:43.78 +57:36:02.2: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 43.78 +57 36 02.2 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458025212355181952,2461199.8322,8.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458025212355181952 20260608.3322 8.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.03 02:37:02.20 +57:41:39.3
136.69003 -2.32907 galactic Cas Second-epoch detections are separated by 2.5" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.2456+57.6870 | 02:37:02.20 +57:41:38.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.198+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:02.20 +57:41:39.3: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:02.20 +57:41:39.3: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 37 02.20 +57 41 39.3 9.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.2456+57.6870,2461199.8322,9.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.2456+57.6870 20260608.3322 9.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.04 02:33:51.00 +55:59:56.1
136.95192 -4.05982 galactic Per Second-epoch detections are separated by 6.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457322349546464896 | 02:33:51.13 +55:59:55.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.763+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:51.00 +55:59:56.1: 12.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:51.00 +55:59:56.1: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 51.00 +55 59 56.1 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457322349546464896,2461199.8322,9.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457322349546464896 20260608.3322 9.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.08 02:30:11.98 +57:38:18.7
135.86661 -2.73169 galactic Per Second-epoch detections are separated by 2.9" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.5502+57.6384 | 02:30:12.05 +57:38:18.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.431+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:11.98 +57:38:18.7: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:11.98 +57:38:18.7: 11.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 11.98 +57 38 18.7 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.5502+57.6384,2461199.8322,9.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.5502+57.6384 20260608.3322 9.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.12 02:21:27.44 +56:16:28.6
135.23901 -4.43097 galactic Per Second-epoch detections are separated by 1.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458256693914103936 | 02:21:27.40 +56:16:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.681+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:27.44 +56:16:28.6: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:27.44 +56:16:28.6: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 27.44 +56 16 28.6 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458256693914103936,2461199.8322,9.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458256693914103936 20260608.3322 9.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.49 01:40:01.08 +60:52:38.4
128.81066 -1.43871 galactic Cas Second-epoch detections are separated by 6.4" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J013956.73+605213.0 | 01:39:56.73 +60:52:13.0 (Gaia DR3) | SR (local) | 450.000000000000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:01.08 +60:52:38.4: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:01.08 +60:52:38.4: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 40 01.08 +60 52 38.4 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J013956.73+605213.0,2461199.8322,9.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J013956.73+605213.0 20260608.3322 9.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.06 02:26:02.37 +56:20:59.5
135.80952 -4.13819 galactic Per Second-epoch detections are separated by 1.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.5102+56.3494 | 02:26:02.46 +56:20:57.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.146+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:02.37 +56:20:59.5: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:02.37 +56:20:59.5: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 02.37 +56 20 59.5 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.5102+56.3494,2461199.8322,9.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.5102+56.3494 20260608.3322 9.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.16 02:24:23.74 +56:54:04.6
135.40150 -3.70292 galactic Per Second-epoch detections are separated by 0.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458386298846823680 | 02:24:18.74 +56:54:02.5 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.768+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:23.74 +56:54:04.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:23.74 +56:54:04.6: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 23.74 +56 54 04.6 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458386298846823680,2461199.8322,9.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458386298846823680 20260608.3322 9.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.12 02:24:38.20 +56:49:55.7
135.45680 -3.75602 galactic Per Second-epoch detections are separated by 1.0" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458384958817070464 | 02:24:38.24 +56:49:54.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.102+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:38.20 +56:49:55.7: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:38.20 +56:49:55.7: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 38.20 +56 49 55.7 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458384958817070464,2461199.8322,9.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458384958817070464 20260608.3322 9.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.07 02:27:52.28 +56:29:28.8
135.99508 -3.91479 galactic Per Second-epoch detections are separated by 1.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457570186338640384 | 02:27:52.24 +56:29:29.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.085+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:52.28 +56:29:28.8: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:52.28 +56:29:28.8: 11.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 52.28 +56 29 28.8 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457570186338640384,2461199.8322,9.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457570186338640384 20260608.3322 9.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.03 02:25:32.87 +56:32:57.7
135.67450 -3.97610 galactic Per Second-epoch detections are separated by 1.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457626261433241088 | 02:25:32.86 +56:32:57.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.674+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:32.87 +56:32:57.7: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:32.87 +56:32:57.7: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 32.87 +56 32 57.7 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457626261433241088,2461199.8322,9.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457626261433241088 20260608.3322 9.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.09 02:22:11.95 +56:20:47.3
135.31121 -4.32818 galactic Per Second-epoch detections are separated by 1.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.5526+56.3433 | 02:22:11.88 +56:20:47.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.152+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:11.95 +56:20:47.3: 12.49 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:11.95 +56:20:47.3: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 11.95 +56 20 47.3 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.5526+56.3433,2461199.8322,9.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.5526+56.3433 20260608.3322 9.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.06 02:33:49.02 +55:57:06.8
136.96582 -4.10499 galactic Per Second-epoch detections are separated by 7.6" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.4666+55.9563 | 02:33:49.36 +55:57:06.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:49.02 +55:57:06.8: 12.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:49.02 +55:57:06.8: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 49.02 +55 57 06.8 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.4666+55.9563,2461199.8322,9.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.4666+55.9563 20260608.3322 9.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.16 02:31:19.72 +56:52:39.5
136.29357 -3.38013 galactic Per Second-epoch detections are separated by 3.0" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.8317+56.8856 | 02:31:19.65 +56:52:39.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.120+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:19.72 +56:52:39.5: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:19.72 +56:52:39.5: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 19.72 +56 52 39.5 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.8317+56.8856,2461199.8322,9.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.8317+56.8856 20260608.3322 9.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.86 02:30:19.30 +55:54:55.0
136.52563 -4.32456 galactic Per Second-epoch detections are separated by 6.3" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457348084991505152 | 02:30:19.49 +55:54:55.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.216+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:19.30 +55:54:55.0: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:19.30 +55:54:55.0: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 19.30 +55 54 55.0 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457348084991505152,2461199.8322,8.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457348084991505152 20260608.3322 8.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.89 02:31:00.30 +56:00:28.1
136.57981 -4.20295 galactic Per Second-epoch detections are separated by 3.6" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457355163097206784 | 02:31:00.46 +56:00:31.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:00.30 +56:00:28.1: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:00.30 +56:00:28.1: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 00.30 +56 00 28.1 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457355163097206784,2461199.8322,8.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457355163097206784 20260608.3322 8.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.11 02:25:11.80 +56:17:22.8
135.72157 -4.23609 galactic Per Second-epoch detections are separated by 3.1" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 457518062614937472 | 02:25:11.71 +56:17:23.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.730+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:11.80 +56:17:22.8: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:11.80 +56:17:22.8: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 11.80 +56 17 22.8 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 457518062614937472,2461199.8322,9.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 457518062614937472 20260608.3322 9.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.09 02:24:18.84 +56:19:49.3
135.59233 -4.24128 galactic Per Second-epoch detections are separated by 1.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.0889+56.3355 | 02:24:18.85 +56:19:48.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.954+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:18.84 +56:19:49.3: 12.43 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:18.84 +56:19:49.3: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 18.84 +56 19 49.3 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.0889+56.3355,2461199.8322,9.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.0889+56.3355 20260608.3322 9.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.12 02:25:48.43 +56:32:35.4
135.71018 -3.96914 galactic Per Second-epoch detections are separated by 1.7" and 8.5 pix
The object was found in VSX10" ZTF J022547.44+563230.2
Type: EW
# Max. Min./Amp. JD0 Period
18.914 g Y 0.532 g 2458358.95060 0.320093600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:48.43 +56:32:35.4: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:48.43 +56:32:35.4: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 48.43 +56 32 35.4 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J022547.44+563230.2,2461199.8322,9.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J022547.44+563230.2 20260608.3322 9.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.18 02:32:04.94 +56:53:51.4
136.38148 -3.32276 galactic Per Second-epoch detections are separated by 1.7" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457966972598282368 | 02:32:05.00 +56:53:49.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.151+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:04.94 +56:53:51.4: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:04.94 +56:53:51.4: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 04.94 +56 53 51.4 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457966972598282368,2461199.8322,9.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457966972598282368 20260608.3322 9.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.04 02:32:35.29 +57:32:20.9
136.20091 -2.70330 galactic Per Second-epoch detections are separated by 1.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.1472+57.5426 | 02:32:35.23 +57:32:21.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1965LS....C05....0H LS V +57 44 J-Ks=0.136+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:35.29 +57:32:20.9: 12.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:35.29 +57:32:20.9: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 35.29 +57 32 20.9 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.1472+57.5426,2461199.8322,9.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.1472+57.5426 20260608.3322 9.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.07 02:30:45.41 +57:06:28.3
136.13471 -3.19597 galactic Per Second-epoch detections are separated by 1.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457984835359661824 | 02:30:45.30 +57:06:29.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.083+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:45.41 +57:06:28.3: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:45.41 +57:06:28.3: 11.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 45.41 +57 06 28.3 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457984835359661824,2461199.8322,9.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457984835359661824 20260608.3322 9.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.20 02:35:26.60 +57:46:11.7
136.46456 -2.34313 galactic Cas Second-epoch detections are separated by 1.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458114925631439104 | 02:35:26.61 +57:46:11.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.609+/-0.026 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:26.60 +57:46:11.7: 10.62 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:26.60 +57:46:11.7: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 35 26.60 +57 46 11.7 9.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458114925631439104,2461199.8322,9.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458114925631439104 20260608.3322 9.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.22 02:23:07.47 +56:41:44.4
135.31016 -3.95640 galactic Per Second-epoch detections are separated by 4.6" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.7879+56.6943 | 02:23:07.31 +56:41:39.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:07.47 +56:41:44.4: 13.24 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:07.47 +56:41:44.4: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 07.47 +56 41 44.4 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.7879+56.6943,2461199.8322,9.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.7879+56.6943 20260608.3322 9.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.10 02:30:51.81 +57:15:44.6
136.09018 -3.04728 galactic Per Second-epoch detections are separated by 0.7" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457992604962793984 | 02:30:51.79 +57:15:44.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.287+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:51.81 +57:15:44.6: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:51.81 +57:15:44.6: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 51.81 +57 15 44.6 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457992604962793984,2461199.8322,9.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457992604962793984 20260608.3322 9.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.22 02:23:08.48 +56:20:24.9
135.43619 -4.28885 galactic Per Second-epoch detections are separated by 0.9" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457527816479322752 | 02:23:08.49 +56:20:25.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.050+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:08.48 +56:20:24.9: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:08.48 +56:20:24.9: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 08.48 +56 20 24.9 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457527816479322752,2461199.8322,9.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457527816479322752 20260608.3322 9.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.17 02:30:16.92 +56:38:09.4
136.25103 -3.65796 galactic Per Second-epoch detections are separated by 0.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457587263129458432 | 02:30:17.01 +56:38:06.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:16.92 +56:38:09.4: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:16.92 +56:38:09.4: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 16.92 +56 38 09.4 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457587263129458432,2461199.8322,9.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457587263129458432 20260608.3322 9.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.14 02:24:52.38 +56:43:10.9
135.52696 -3.84978 galactic Per Second-epoch detections are separated by 2.4" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457632652344319616 | 02:24:52.42 +56:43:10.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.731+/-0.029 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:52.38 +56:43:10.9: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:52.38 +56:43:10.9: 11.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 52.38 +56 43 10.9 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457632652344319616,2461199.8322,9.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457632652344319616 20260608.3322 9.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.30 02:35:34.92 +57:32:59.3
136.56773 -2.53849 galactic Per Second-epoch detections are separated by 2.6" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.8988+57.5514 | 02:35:35.71 +57:33:05.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:34.92 +57:32:59.3: 11.75 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:34.92 +57:32:59.3: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 35 34.92 +57 32 59.3 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.8988+57.5514,2461199.8322,9.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.8988+57.5514 20260608.3322 9.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.99 02:28:32.01 +56:00:36.5
136.25731 -4.32904 galactic Per Second-epoch detections are separated by 5.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457539537452434560 | 02:28:32.37 +56:00:37.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:32.01 +56:00:36.5: 12.81 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:32.01 +56:00:36.5: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 28 32.01 +56 00 36.5 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457539537452434560,2461199.8322,8.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457539537452434560 20260608.3322 8.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.27 02:24:53.93 +56:08:45.2
135.73386 -4.38521 galactic Per Second-epoch detections are separated by 1.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.2276+56.1492 | 02:24:53.87 +56:08:46.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.132+/-0.034 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:53.93 +56:08:45.2: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:53.93 +56:08:45.2: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 53.93 +56 08 45.2 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.2276+56.1492,2461199.8322,9.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.2276+56.1492 20260608.3322 9.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.16 02:27:34.40 +56:16:53.2
136.03314 -4.12530 galactic Per Second-epoch detections are separated by 1.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.8823+56.2862 | 02:27:34.40 +56:16:53.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.111+/-0.025 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:34.40 +56:16:53.2: 11.13 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:34.40 +56:16:53.2: 11.74 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 34.40 +56 16 53.2 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.8823+56.2862,2461199.8322,9.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.8823+56.2862 20260608.3322 9.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.21 02:36:55.81 +57:38:49.8
136.69560 -2.37794 galactic Cas Second-epoch detections are separated by 3.1" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.2323+57.6467 | 02:36:55.77 +57:38:48.4 (Gaia DR3) | LPV (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.185+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:55.81 +57:38:49.8: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:55.81 +57:38:49.8: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 36 55.81 +57 38 49.8 9.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.2323+57.6467,2461199.8322,9.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.2323+57.6467 20260608.3322 9.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.03 02:34:12.97 +56:11:54.0
136.92194 -3.85615 galactic Per Second-epoch detections are separated by 7.2" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457326232196815232 | 02:34:13.32 +56:12:39.2 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE J-Ks=0.127+/-0.030 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:12.97 +56:11:54.0: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:12.97 +56:11:54.0: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 12.97 +56 11 54.0 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457326232196815232,2461199.8322,9.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457326232196815232 20260608.3322 9.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.28 02:20:11.71 +56:22:22.8
135.04045 -4.39780 galactic Per Second-epoch detections are separated by 2.3" and 8.4 pix
The object was found in VSX11" ZTF J022010.56+562228.1
Type: EW
# Max. Min./Amp. JD0 Period
17.880 r Y 0.223 r 2458303.96760 0.419228000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:11.71 +56:22:22.8: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:11.71 +56:22:22.8: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 20 11.71 +56 22 22.8 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J022010.56+562228.1,2461199.8322,9.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J022010.56+562228.1 20260608.3322 9.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.19 02:29:55.64 +56:55:49.6
136.09606 -3.40269 galactic Per Second-epoch detections are separated by 0.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.4814+56.9308 | 02:29:55.55 +56:55:50.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1965LS....C05....0H LS V +56 50 J-Ks=0.125+/-0.063 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:55.64 +56:55:49.6: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:55.64 +56:55:49.6: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 55.64 +56 55 49.6 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.4814+56.9308,2461199.8322,9.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.4814+56.9308 20260608.3322 9.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.28 02:30:33.48 +56:57:02.6
136.16844 -3.35183 galactic Per Second-epoch detections are separated by 0.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457978929787415936 | 02:30:33.42 +56:57:02.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.162+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:33.48 +56:57:02.6: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:33.48 +56:57:02.6: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 33.48 +56 57 02.6 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457978929787415936,2461199.8322,9.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457978929787415936 20260608.3322 9.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.08 02:31:03.43 +55:52:01.6
136.63960 -4.33060 galactic Per Second-epoch detections are separated by 4.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457340938165655808 | 02:31:03.60 +55:52:02.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.294+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:03.43 +55:52:01.6: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:03.43 +55:52:01.6: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 03.43 +55 52 01.6 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457340938165655808,2461199.8322,9.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457340938165655808 20260608.3322 9.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.46 02:20:25.25 +56:52:28.8
134.90003 -3.91508 galactic Per Second-epoch detections are separated by 5.8" and 8.9 pix
The object was found in VSX 8" Gaia DR3 458350839599353088
Type: ROT
# Max. Min./Amp. JD0 Period
15.880 G 15.920 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:25.25 +56:52:28.8: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:25.25 +56:52:28.8: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 20 25.25 +56 52 28.8 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458350839599353088,2461199.8322,9.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458350839599353088 20260608.3322 9.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.29 02:23:11.37 +56:11:21.3
135.49515 -4.42810 galactic Per Second-epoch detections are separated by 2.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.7975+56.1884 | 02:23:11.42 +56:11:18.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:11.37 +56:11:21.3: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:11.37 +56:11:21.3: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 11.37 +56 11 21.3 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.7975+56.1884,2461199.8322,9.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.7975+56.1884 20260608.3322 9.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.29 02:26:55.66 +56:28:24.5
135.87988 -3.97869 galactic Per Second-epoch detections are separated by 2.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.7308+56.4791 | 02:26:56.13 +56:28:21.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:55.66 +56:28:24.5: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:55.66 +56:28:24.5: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 55.66 +56 28 24.5 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.7308+56.4791,2461199.8322,9.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.7308+56.4791 20260608.3322 9.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.30 02:22:16.04 +56:22:42.6
135.30903 -4.29486 galactic Per Second-epoch detections are separated by 2.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458278203113550720 | 02:22:15.95 +56:22:42.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.043+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:16.04 +56:22:42.6: 13.04 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:16.04 +56:22:42.6: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 16.04 +56 22 42.6 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458278203113550720,2461199.8322,9.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458278203113550720 20260608.3322 9.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.31 02:27:23.12 +56:19:27.5
135.99317 -4.09483 galactic Per Second-epoch detections are separated by 3.0" and 8.8 pix
The object was found in VSX 2" Gaia DR3 457562214879587968
Type: BE|GCAS|S
# Max. Min./Amp. JD0 Period
11.540 G 11.620 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:23.12 +56:19:27.5: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:23.12 +56:19:27.5: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 23.12 +56 19 27.5 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457562214879587968,2461199.8322,9.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457562214879587968 20260608.3322 9.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.36 02:33:27.67 +57:14:45.0
136.42195 -2.92940 galactic Per Second-epoch detections are separated by 2.6" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458001847733355264 | 02:33:27.56 +57:14:44.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.304+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:27.67 +57:14:45.0: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:27.67 +57:14:45.0: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 27.67 +57 14 45.0 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458001847733355264,2461199.8322,9.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458001847733355264 20260608.3322 9.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.40 02:24:46.87 +56:38:55.3
135.54029 -3.92066 galactic Per Second-epoch detections are separated by 0.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457630895694121216 | 02:24:46.83 +56:38:55.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.327+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:46.87 +56:38:55.3: 11.49 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:46.87 +56:38:55.3: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 46.87 +56 38 55.3 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457630895694121216,2461199.8322,9.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457630895694121216 20260608.3322 9.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.15 02:29:39.11 +56:11:33.0
136.33519 -4.10202 galactic Per Second-epoch detections are separated by 3.2" and 8.2 pix
The object was found in VSX 6" NSV 15519
Type: SR
# Max. Min./Amp. JD0 Period
12.400 V 13.100 V 2458443.36190 299.178129200000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:39.11 +56:11:33.0: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:39.11 +56:11:33.0: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 39.11 +56 11 33.0 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 15519,2461199.8322,9.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 15519 20260608.3322 9.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.43 02:37:01.15 +57:51:23.0
136.62363 -2.18111 galactic Cas Second-epoch detections are separated by 1.0" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458136847144779648 | 02:37:01.18 +57:51:21.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.154+/-0.037 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:01.15 +57:51:23.0: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:01.15 +57:51:23.0: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 37 01.15 +57 51 23.0 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458136847144779648,2461199.8322,9.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458136847144779648 20260608.3322 9.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.31 02:32:23.31 +57:38:37.3
136.13634 -2.61677 galactic Per Second-epoch detections are separated by 1.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458074312422945920 | 02:32:23.20 +57:38:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1IV (LAMOST DR5) J-Ks=1.170+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:23.31 +57:38:37.3: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:23.31 +57:38:37.3: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 23.31 +57 38 37.3 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458074312422945920,2461199.8322,9.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458074312422945920 20260608.3322 9.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.27 02:24:38.57 +56:20:45.4
135.62958 -4.21064 galactic Per Second-epoch detections are separated by 2.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.1775+56.3470 | 02:24:38.69 +56:20:47.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.310+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:38.57 +56:20:45.4: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:38.57 +56:20:45.4: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 38.57 +56 20 45.4 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.1775+56.3470,2461199.8322,9.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.1775+56.3470 20260608.3322 9.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.30 02:30:35.00 +56:43:58.4
136.25323 -3.55258 galactic Per Second-epoch detections are separated by 4.5" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457589565231823360 | 02:30:35.06 +56:43:56.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.926+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:35.00 +56:43:58.4: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:35.00 +56:43:58.4: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 35.00 +56 43 58.4 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457589565231823360,2461199.8322,9.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457589565231823360 20260608.3322 9.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.30 02:31:51.45 +56:45:51.1
136.40357 -3.45789 galactic Per Second-epoch detections are separated by 2.3" and 8.5 pix
The object was found in VSX 6" NSV 15534
Type: LB:
# Max. Min./Amp. JD0 Period
12.900 V 13.200 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:51.45 +56:45:51.1: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:51.45 +56:45:51.1: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 51.45 +56 45 51.1 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 15534,2461199.8322,9.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 15534 20260608.3322 9.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.36 02:32:55.48 +57:08:54.0
136.39211 -3.04729 galactic Per Second-epoch detections are separated by 1.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457999648710144000 | 02:32:55.50 +57:08:53.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.889+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:55.48 +57:08:54.0: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:55.48 +57:08:54.0: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 55.48 +57 08 54.0 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457999648710144000,2461199.8322,9.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457999648710144000 20260608.3322 9.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.14 02:34:13.94 +56:18:42.0
136.88008 -3.75077 galactic Per Second-epoch detections are separated by 6.7" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457749097496685824 | 02:34:14.13 +56:18:41.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.801+/-0.041 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:13.94 +56:18:42.0: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:13.94 +56:18:42.0: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 13.94 +56 18 42.0 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457749097496685824,2461199.8322,9.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457749097496685824 20260608.3322 9.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.34 02:29:11.28 +57:21:01.0
135.84712 -3.04978 galactic Per Second-epoch detections are separated by 2.3" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458038745789149824 | 02:29:11.20 +57:20:59.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.788+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:11.28 +57:21:01.0: 12.69 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:11.28 +57:21:01.0: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 11.28 +57 21 01.0 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458038745789149824,2461199.8322,9.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458038745789149824 20260608.3322 9.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.34 02:27:53.71 +57:06:30.9
135.77281 -3.33877 galactic Per Second-epoch detections are separated by 0.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457670276258952448 | 02:27:53.69 +57:06:31.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1965LS....C05....0H LS V +56 47 J-Ks=0.125+/-0.030 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:53.71 +57:06:30.9: 12.69 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:53.71 +57:06:30.9: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 53.71 +57 06 30.9 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457670276258952448,2461199.8322,9.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457670276258952448 20260608.3322 9.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.31 02:32:01.27 +56:51:17.5
136.38996 -3.36549 galactic Per Second-epoch detections are separated by 1.9" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.0170+56.8475 | 02:32:01.27 +56:51:18.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.307+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:01.27 +56:51:17.5: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:01.27 +56:51:17.5: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 01.27 +56 51 17.5 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.0170+56.8475,2461199.8322,9.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.0170+56.8475 20260608.3322 9.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.38 02:33:37.69 +57:40:25.1
136.27826 -2.52576 galactic Per Second-epoch detections are separated by 2.9" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.4074+57.6734 | 02:33:40.23 +57:40:02.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.496+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:37.69 +57:40:25.1: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:37.69 +57:40:25.1: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 37.69 +57 40 25.1 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.4074+57.6734,2461199.8322,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.4074+57.6734 20260608.3322 9.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.16 00:43:47.78 +61:53:59.7
122.03210 -0.95848 galactic Cas Second-epoch detections are separated by 1.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 427618218288011776 | 00:43:43.86 +61:53:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1991AJ....102..177L Cl* NGC 225 LMM 104 J-Ks=0.506+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:43:47.78 +61:53:59.7: 12.43 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:43:47.78 +61:53:59.7: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 00 43 47.78 +61 53 59.7 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 427618218288011776,2461199.8322,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 427618218288011776 20260608.3322 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.36 02:32:47.65 +57:14:17.2
136.34143 -2.97105 galactic Per Second-epoch detections are separated by 0.9" and 8.4 pix
The object was found in VSX23" ZTF J023246.55+571356.5
Type: RS
# Max. Min./Amp. JD0 Period
16.972 r Y 0.150 r 2458486.65480 4.402844100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:47.65 +57:14:17.2: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:47.65 +57:14:17.2: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 47.65 +57 14 17.2 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J023246.55+571356.5,2461199.8322,9.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J023246.55+571356.5 20260608.3322 9.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.43 02:22:21.43 +56:34:19.1
135.25385 -4.10897 galactic Per Second-epoch detections are separated by 1.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.6108+56.5718 | 02:22:21.39 +56:34:19.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.149+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:21.43 +56:34:19.1: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:21.43 +56:34:19.1: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 21.43 +56 34 19.1 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.6108+56.5718,2461199.8322,9.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.6108+56.5718 20260608.3322 9.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.24 02:32:49.40 +57:34:21.9
136.21728 -2.66021 galactic Per Second-epoch detections are separated by 0.1" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.2179+57.5617 | 02:32:49.16 +57:34:21.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.222+/-0.039 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:49.40 +57:34:21.9: 10.42 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:49.40 +57:34:21.9: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 49.40 +57 34 21.9 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.2179+57.5617,2461199.8322,9.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.2179+57.5617 20260608.3322 9.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.45 02:20:54.28 +56:36:05.4
135.05534 -4.14964 galactic Per Second-epoch detections are separated by 1.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458296070174692608 | 02:20:54.38 +56:36:05.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.774+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:54.28 +56:36:05.4: 12.96 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:54.28 +56:36:05.4: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 20 54.28 +56 36 05.4 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458296070174692608,2461199.8322,9.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458296070174692608 20260608.3322 9.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.45 02:22:22.77 +56:40:00.7
135.22394 -4.01884 galactic Per Second-epoch detections are separated by 2.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458291362890696832 | 02:22:22.82 +56:40:01.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.912+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:22.77 +56:40:00.7: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:22.77 +56:40:00.7: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 22.77 +56 40 00.7 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458291362890696832,2461199.8322,9.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458291362890696832 20260608.3322 9.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.38 02:27:27.07 +56:31:10.2
135.93069 -3.90963 galactic Per Second-epoch detections are separated by 2.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457617327901248128 | 02:27:27.12 +56:31:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.405+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:27.07 +56:31:10.2: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:27.07 +56:31:10.2: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 27.07 +56 31 10.2 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457617327901248128,2461199.8322,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457617327901248128 20260608.3322 9.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.47 02:21:52.46 +56:32:45.3
135.20021 -4.15631 galactic Per Second-epoch detections are separated by 4.6" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458284555357304704 | 02:21:52.39 +56:32:45.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.302+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:52.46 +56:32:45.3: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:52.46 +56:32:45.3: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 52.46 +56 32 45.3 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458284555357304704,2461199.8322,9.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458284555357304704 20260608.3322 9.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.43 02:24:12.53 +56:49:25.8
135.40483 -3.78440 galactic Per Second-epoch detections are separated by 0.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.0445+56.8257 | 02:24:12.46 +56:49:26.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.242+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:12.53 +56:49:25.8: 12.66 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:12.53 +56:49:25.8: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 12.53 +56 49 25.8 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.0445+56.8257,2461199.8322,9.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.0445+56.8257 20260608.3322 9.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.36 02:21:33.10 +56:13:41.1
135.26732 -4.47021 galactic Per Second-epoch detections are separated by 2.9" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.3809+56.2181 | 02:21:32.94 +56:13:40.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.082+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:33.10 +56:13:41.1: 10.35 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:33.10 +56:13:41.1: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 33.10 +56 13 41.1 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.3809+56.2181,2461199.8322,9.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.3809+56.2181 20260608.3322 9.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.43 02:25:40.03 +56:29:20.6
135.71146 -4.02658 galactic Per Second-epoch detections are separated by 2.4" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 457614098080789120 | 02:25:39.98 +56:29:20.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.784+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:40.03 +56:29:20.6: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:40.03 +56:29:20.6: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 40.03 +56 29 20.6 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 457614098080789120,2461199.8322,9.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 457614098080789120 20260608.3322 9.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.57 02:21:38.53 +56:26:50.2
135.20392 -4.25996 galactic Per Second-epoch detections are separated by 2.4" and 8.3 pix
The object was found in VSX 3" ASASSN-V J022138.78+562648.0
Type: SR
# Max. Min./Amp. JD0 Period
14.200 g Y 0.390 g 2458438.85200 90.140000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:38.53 +56:26:50.2: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:38.53 +56:26:50.2: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 38.53 +56 26 50.2 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J022138.78+562648.0,2461199.8322,9.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J022138.78+562648.0 20260608.3322 9.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.45 02:26:14.40 +56:12:13.5
135.88807 -4.26463 galactic Per Second-epoch detections are separated by 2.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457467004044691712 | 02:26:14.28 +56:12:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.140+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:14.40 +56:12:13.5: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:14.40 +56:12:13.5: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 14.40 +56 12 13.5 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457467004044691712,2461199.8322,9.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457467004044691712 20260608.3322 9.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.44 02:39:23.99 +58:09:11.5
136.79402 -1.78294 galactic Cas Second-epoch detections are separated by 4.6" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.8494+58.1525 | 02:39:23.88 +58:09:09.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1959LS....C01....0H LS I +57 78 J-Ks=0.217+/-0.027 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:39:23.99 +58:09:11.5: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:39:23.99 +58:09:11.5: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 39 23.99 +58 09 11.5 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.8494+58.1525,2461199.8322,9.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.8494+58.1525 20260608.3322 9.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.36 02:36:41.37 +57:37:08.5
136.67712 -2.41652 galactic Cas Second-epoch detections are separated by 2.3" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.1865+57.6232 | 02:36:41.37 +57:37:09.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.293+/-0.026 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:41.37 +57:37:08.5: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:41.37 +57:37:08.5: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 36 41.37 +57 37 08.5 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.1865+57.6232,2461199.8322,9.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.1865+57.6232 20260608.3322 9.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.43 02:35:58.35 +57:49:15.3
136.50951 -2.26860 galactic Cas Second-epoch detections are separated by 1.5" and 8.4 pix
The object was found in VSX23" Gaia DR3 458116196941724800
Type: ROT
# Max. Min./Amp. JD0 Period
17.300 G 17.400 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:58.35 +57:49:15.3: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:58.35 +57:49:15.3: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 35 58.35 +57 49 15.3 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458116196941724800,2461199.8322,9.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458116196941724800 20260608.3322 9.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.49 02:39:21.42 +58:07:09.8
136.80251 -1.81614 galactic Cas Second-epoch detections are separated by 1.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 463964220109550080 | 02:39:21.53 +58:07:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.935+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:39:21.42 +58:07:09.8: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:39:21.42 +58:07:09.8: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 39 21.42 +58 07 09.8 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 463964220109550080,2461199.8322,9.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 463964220109550080 20260608.3322 9.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.51 02:29:41.54 +56:37:30.7
136.17960 -3.69809 galactic Per Second-epoch detections are separated by 1.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457593379162918784 | 02:29:41.70 +56:37:31.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.191+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:41.54 +56:37:30.7: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:41.54 +56:37:30.7: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 41.54 +56 37 30.7 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457593379162918784,2461199.8322,9.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457593379162918784 20260608.3322 9.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.93 00:58:55.93 +58:04:05.2
123.92621 -4.78917 galactic Cas Second-epoch detections are separated by 1.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:58:55.93 +58:04:05.2 (user input) | T | P | (position from user input) J-Ks=0.236+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:58:55.93 +58:04:05.2: 12.18 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:58:55.93 +58:04:05.2: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 00 58 55.93 +58 04 05.2 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.46 02:33:30.94 +57:29:02.8
136.33718 -2.70655 galactic Per Second-epoch detections are separated by 2.4" and 8.8 pix
The object was found in VSX 1" Gaia23dql
Type: GCAS
# Max. Min./Amp. JD0 Period
11.590 G 11.980 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:30.94 +57:29:02.8: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:30.94 +57:29:02.8: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 30.94 +57 29 02.8 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia23dql,2461199.8322,9.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia23dql 20260608.3322 9.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.38 02:22:47.76 +56:11:09.8
135.44477 -4.45010 galactic Per Second-epoch detections are separated by 0.7" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.7007+56.1904 | 02:22:47.64 +56:11:09.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.443+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:47.76 +56:11:09.8: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:47.76 +56:11:09.8: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 47.76 +56 11 09.8 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.7007+56.1904,2461199.8322,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.7007+56.1904 20260608.3322 9.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.55 02:21:19.11 +56:38:13.4
135.09687 -4.09684 galactic Per Second-epoch detections are separated by 3.6" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.3292+56.6370 | 02:21:19.02 +56:38:13.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.798+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:19.11 +56:38:13.4: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:19.11 +56:38:13.4: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 19.11 +56 38 13.4 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.3292+56.6370,2461199.8322,9.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.3292+56.6370 20260608.3322 9.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.60 02:17:41.08 +56:28:32.5
134.67788 -4.41639 galactic Per Second-epoch detections are separated by 2.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J034.4215+56.4760 | 02:17:41.17 +56:28:33.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.212+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:17:41.08 +56:28:32.5: 11.48 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:17:41.08 +56:28:32.5: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 17 41.08 +56 28 32.5 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J034.4215+56.4760,2461199.8322,9.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J034.4215+56.4760 20260608.3322 9.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.51 02:28:01.17 +56:23:28.1
136.05082 -4.00062 galactic Per Second-epoch detections are separated by 1.0" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.9932+56.3960 | 02:28:00.52 +56:23:27.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:01.17 +56:23:28.1: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:01.17 +56:23:28.1: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 28 01.17 +56 23 28.1 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.9932+56.3960,2461199.8322,9.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.9932+56.3960 20260608.3322 9.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.49 02:21:16.36 +56:23:43.0
135.17358 -4.32628 galactic Per Second-epoch detections are separated by 3.0" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458258411900977280 | 02:21:16.26 +56:23:43.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.037+/-0.034 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:16.36 +56:23:43.0: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:16.36 +56:23:43.0: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 16.36 +56 23 43.0 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458258411900977280,2461199.8322,9.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458258411900977280 20260608.3322 9.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.62 02:24:58.44 +56:50:40.4
135.49565 -3.72810 galactic Per Second-epoch detections are separated by 4.5" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457640314566066688 | 02:24:58.37 +56:50:38.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.932+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:58.44 +56:50:40.4: 13.22 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:58.44 +56:50:40.4: 12.46 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 58.44 +56 50 40.4 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457640314566066688,2461199.8322,9.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457640314566066688 20260608.3322 9.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.57 02:25:52.54 +57:02:04.3
135.54313 -3.50682 galactic Per Second-epoch detections are separated by 2.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457666634126204032 | 02:25:52.40 +57:02:03.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.758+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:52.54 +57:02:04.3: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:52.54 +57:02:04.3: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 52.54 +57 02 04.3 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457666634126204032,2461199.8322,9.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457666634126204032 20260608.3322 9.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.35 02:27:42.18 +56:12:19.8
136.07765 -4.18949 galactic Per Second-epoch detections are separated by 3.7" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457557713753714944 | 02:27:42.19 +56:12:18.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.386+/-0.029 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:42.18 +56:12:19.8: 12.95 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:42.18 +56:12:19.8: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 42.18 +56 12 19.8 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457557713753714944,2461199.8322,9.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457557713753714944 20260608.3322 9.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.59 02:23:54.58 +56:06:52.8
135.61552 -4.46297 galactic Per Second-epoch detections are separated by 3.1" and 8.6 pix
The object was found in VSX25" ZTF J022354.02+560717.1
Type: EA
# Max. Min./Amp. JD0 Period
20.588 r Y 0.819 r 2458483.61410 0.277178600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:54.58 +56:06:52.8: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:54.58 +56:06:52.8: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 54.58 +56 06 52.8 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J022354.02+560717.1,2461199.8322,9.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J022354.02+560717.1 20260608.3322 9.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.86 01:58:16.63 +59:38:57.1
131.29149 -2.13333 galactic Cas Second-epoch detections are separated by 5.8" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:58:16.63 +59:38:57.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:16.63 +59:38:57.1: 12.68 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:16.63 +59:38:57.1: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 58 16.63 +59 38 57.1 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,9.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 9.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.61 02:31:45.84 +57:14:33.1
136.21065 -3.01986 galactic Per Second-epoch detections are separated by 2.8" and 8.3 pix
The object was found in VSX 3" ASASSN-V J023146.20+571431.6
Type: L
# Max. Min./Amp. JD0 Period
13.250 V 13.610 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:45.84 +57:14:33.1: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:45.84 +57:14:33.1: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 45.84 +57 14 33.1 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J023146.20+571431.6,2461199.8322,9.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J023146.20+571431.6 20260608.3322 9.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.56 02:17:50.40 +56:22:37.9
134.73067 -4.50238 galactic Per Second-epoch detections are separated by 1.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J034.4666+56.3877 | 02:17:50.40 +56:22:40.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.874+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:17:50.40 +56:22:37.9: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:17:50.40 +56:22:37.9: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 17 50.40 +56 22 37.9 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J034.4666+56.3877,2461199.8322,9.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J034.4666+56.3877 20260608.3322 9.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.47 02:21:13.54 +56:28:44.7
135.13881 -4.24971 galactic Per Second-epoch detections are separated by 5.3" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458294146029662208 | 02:21:13.36 +56:28:43.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.313+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:13.54 +56:28:44.7: 12.95 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:13.54 +56:28:44.7: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 13.54 +56 28 44.7 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458294146029662208,2461199.8322,9.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458294146029662208 20260608.3322 9.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.62 02:24:21.26 +56:52:14.7
135.40697 -3.73348 galactic Per Second-epoch detections are separated by 3.5" and 8.8 pix
The object was found in VSX 1" Gaia DR3 458386054022555648
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.250 G 12.310 G 4.320920000000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:21.26 +56:52:14.7: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:21.26 +56:52:14.7: 12.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 21.26 +56 52 14.7 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458386054022555648,2461199.8322,9.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458386054022555648 20260608.3322 9.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.59 02:24:38.41 +56:48:43.1
135.46438 -3.77472 galactic Per Second-epoch detections are separated by 1.4" and 8.3 pix
The object was found in VSX10" Gaia DR3 458384787018395520
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.810 G 13.840 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:38.41 +56:48:43.1: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:38.41 +56:48:43.1: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 38.41 +56 48 43.1 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458384787018395520,2461199.8322,9.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458384787018395520 20260608.3322 9.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.53 02:34:31.90 +57:40:30.4
136.38923 -2.47781 galactic Per Second-epoch detections are separated by 2.7" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458118877000959872 | 02:34:32.11 +57:40:33.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:31.90 +57:40:30.4: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:31.90 +57:40:30.4: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 31.90 +57 40 30.4 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458118877000959872,2461199.8322,9.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458118877000959872 20260608.3322 9.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.57 02:26:01.02 +56:28:14.9
135.76321 -4.02637 galactic Per Second-epoch detections are separated by 4.1" and 8.0 pix
The object was found in VSX 3" Gaia DR3 457613342171654272
Type: VAR
# Max. Min./Amp. JD0 Period
12.120 G 12.140 G 0.249219000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:01.02 +56:28:14.9: 12.66 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:01.02 +56:28:14.9: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 01.02 +56 28 14.9 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457613342171654272,2461199.8322,9.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457613342171654272 20260608.3322 9.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.44 02:23:57.17 +56:11:53.7
135.59178 -4.38259 galactic Per Second-epoch detections are separated by 2.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.9838+56.2016 | 02:23:57.00 +56:11:54.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.131+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:57.17 +56:11:53.7: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:57.17 +56:11:53.7: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 57.17 +56 11 53.7 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.9838+56.2016,2461199.8322,9.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.9838+56.2016 20260608.3322 9.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.09 01:29:32.95 +61:46:25.0
127.42242 -0.76540 galactic Cas Second-epoch detections are separated by 0.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:29:32.95 +61:46:25.0 (user input) | T | P | (position from user input) J-Ks=0.908+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:32.95 +61:46:25.0: 12.95 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:32.95 +61:46:25.0: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 29 32.95 +61 46 25.0 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.56 02:34:04.49 +57:32:44.3
136.38285 -2.62086 galactic Per Second-epoch detections are separated by 4.9" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.5396+57.5452 | 02:34:04.33 +57:32:39.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:04.49 +57:32:44.3: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:04.49 +57:32:44.3: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 04.49 +57 32 44.3 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.5396+57.5452,2461199.8322,9.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.5396+57.5452 20260608.3322 9.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.65 02:36:12.26 +57:41:56.0
136.58593 -2.36868 galactic Cas Second-epoch detections are separated by 1.3" and 8.7 pix
The object was found in VSX 3" Gaia DR3 458111038678203904
Type: ROT
# Max. Min./Amp. JD0 Period
12.370 G 12.390 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:12.26 +57:41:56.0: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:12.26 +57:41:56.0: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 36 12.26 +57 41 56.0 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458111038678203904,2461199.8322,9.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458111038678203904 20260608.3322 9.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.51 02:28:09.05 +56:38:21.2
135.97693 -3.76305 galactic Per Second-epoch detections are separated by 2.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.0372+56.6387 | 02:28:08.94 +56:38:19.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.192+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:09.05 +56:38:21.2: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:09.05 +56:38:21.2: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 28 09.05 +56 38 21.2 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.0372+56.6387,2461199.8322,9.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.0372+56.6387 20260608.3322 9.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.05 01:18:14.29 +61:44:36.0
126.09871 -0.96352 galactic Cas Second-epoch detections are separated by 1.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:18:14.29 +61:44:36.0 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:14.29 +61:44:36.0: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:14.29 +61:44:36.0: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 18 14.29 +61 44 36.0 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.41 02:31:47.11 +55:52:28.5
136.73162 -4.28516 galactic Per Second-epoch detections are separated by 3.1" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457338876581619456 | 02:31:47.43 +55:52:29.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:47.11 +55:52:28.5: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:47.11 +55:52:28.5: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 47.11 +55 52 28.5 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457338876581619456,2461199.8322,9.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457338876581619456 20260608.3322 9.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.52 02:27:22.05 +56:31:18.8
135.91904 -3.91159 galactic Per Second-epoch detections are separated by 4.1" and 8.7 pix
The object was found in VSX21" ZTF J022719.47+563119.0
Type: HADS
# Max. Min./Amp. JD0 Period
18.002 r Y 0.199 r 2458428.78930 0.077707800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:22.05 +56:31:18.8: 13.02 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:22.05 +56:31:18.8: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 22.05 +56 31 18.8 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J022719.47+563119.0,2461199.8322,9.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J022719.47+563119.0 20260608.3322 9.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.52 02:37:15.58 +57:48:19.2
136.67329 -2.21529 galactic Cas Second-epoch detections are separated by 2.2" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458135743330088064 | 02:37:15.63 +57:48:20.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.713+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:15.58 +57:48:19.2: 11.69 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:15.58 +57:48:19.2: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 37 15.58 +57 48 19.2 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458135743330088064,2461199.8322,9.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458135743330088064 20260608.3322 9.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.63 02:21:39.29 +56:31:44.8
135.17748 -4.18247 galactic Per Second-epoch detections are separated by 1.9" and 8.3 pix
The object was found in VSX25" Gaia DR3 458283013474392320
Type: ROT
# Max. Min./Amp. JD0 Period
15.560 G 15.620 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:39.29 +56:31:44.8: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:39.29 +56:31:44.8: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 39.29 +56 31 44.8 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458283013474392320,2461199.8322,9.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458283013474392320 20260608.3322 9.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.45 02:33:11.11 +57:33:48.8
136.26568 -2.65017 galactic Per Second-epoch detections are separated by 0.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458023494368301824 | 02:33:11.18 +57:33:50.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.177+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:11.11 +57:33:48.8: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:11.11 +57:33:48.8: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 11.11 +57 33 48.8 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458023494368301824,2461199.8322,9.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458023494368301824 20260608.3322 9.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.64 02:23:43.00 +56:38:37.8
135.40470 -3.97663 galactic Per Second-epoch detections are separated by 3.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.9286+56.6441 | 02:23:42.88 +56:38:38.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.179+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:43.00 +56:38:37.8: 12.34 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:43.00 +56:38:37.8: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 43.00 +56 38 37.8 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.9286+56.6441,2461199.8322,9.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.9286+56.6441 20260608.3322 9.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.65 02:20:52.81 +56:09:33.8
135.20272 -4.56663 galactic Per Second-epoch detections are separated by 0.5" and 8.1 pix
The object was found in VSX24" Gaia DR3 458248619375657088
Type: E
# Max. Min./Amp. JD0 Period
13.910 G 14.230 G 5.797200000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:52.81 +56:09:33.8: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:52.81 +56:09:33.8: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 20 52.81 +56 09 33.8 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458248619375657088,2461199.8322,9.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458248619375657088 20260608.3322 9.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.54 02:34:19.87 +57:08:33.3
136.57067 -2.97928 galactic Per Second-epoch detections are separated by 2.5" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457809635051571200 | 02:34:20.02 +57:08:33.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.760+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:19.87 +57:08:33.3: 11.92 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:19.87 +57:08:33.3: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 19.87 +57 08 33.3 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457809635051571200,2461199.8322,9.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457809635051571200 20260608.3322 9.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.31 00:36:55.91 +62:32:56.0
121.26098 -0.27579 galactic Cas Second-epoch detections are separated by 5.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 430697366244614272 | 00:37:00.66 +62:32:35.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1956PMcCO..13a....B AG+62 73
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:36:55.91 +62:32:56.0: 12.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:36:55.91 +62:32:56.0: 13.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 00 36 55.91 +62 32 56.0 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 430697366244614272,2461199.8322,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430697366244614272 20260608.3322 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.62 02:30:17.43 +56:43:02.2
136.22173 -3.58206 galactic Per Second-epoch detections are separated by 4.1" and 8.4 pix
The object was found in VSX 3" Gaia DR3 457599838793614592
Type: VAR
# Max. Min./Amp. JD0 Period
12.180 G 12.200 G 0.027789200000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:17.43 +56:43:02.2: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:17.43 +56:43:02.2: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 17.43 +56 43 02.2 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457599838793614592,2461199.8322,9.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457599838793614592 20260608.3322 9.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.63 02:28:44.08 +57:00:25.5
135.91640 -3.39150 galactic Per Second-epoch detections are separated by 0.7" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457655497265270528 | 02:28:44.14 +57:00:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.764+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:44.08 +57:00:25.5: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:44.08 +57:00:25.5: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 28 44.08 +57 00 25.5 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457655497265270528,2461199.8322,9.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457655497265270528 20260608.3322 9.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.62 02:31:18.74 +57:03:50.9
136.22120 -3.20818 galactic Per Second-epoch detections are separated by 2.2" and 8.7 pix
The object was found in VSX 4" Gaia DR3 457981403688250240
Type: ROT
# Max. Min./Amp. JD0 Period
12.410 G 12.440 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:18.74 +57:03:50.9: 13.08 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:18.74 +57:03:50.9: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 18.74 +57 03 50.9 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457981403688250240,2461199.8322,9.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457981403688250240 20260608.3322 9.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.74 02:18:56.21 +56:18:32.0
134.89719 -4.51660 galactic Per Second-epoch detections are separated by 1.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:18:56.21 +56:18:32.0 (user input) | T | P | (position from user input) J-Ks=0.608+/-0.036 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:56.21 +56:18:32.0: 12.59 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:56.21 +56:18:32.0: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 18 56.21 +56 18 32.0 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 9.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.61 02:29:08.36 +57:12:16.0
135.89484 -3.18776 galactic Per Second-epoch detections are separated by 0.4" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.2786+57.2059 | 02:29:08.33 +57:12:15.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.098+/-0.034 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:08.36 +57:12:16.0: 12.81 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:08.36 +57:12:16.0: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 08.36 +57 12 16.0 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.2786+57.2059,2461199.8322,9.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.2786+57.2059 20260608.3322 9.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.74 02:23:53.85 +56:39:14.7
135.42444 -3.95834 galactic Per Second-epoch detections are separated by 1.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458382068296388352 | 02:23:53.86 +56:39:14.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.826+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:53.85 +56:39:14.7: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:53.85 +56:39:14.7: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 53.85 +56 39 14.7 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458382068296388352,2461199.8322,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458382068296388352 20260608.3322 9.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.48 02:30:51.42 +57:16:48.8
136.08267 -3.03107 galactic Per Second-epoch detections are separated by 0.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457992703739740416 | 02:30:51.33 +57:16:48.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.235+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:51.42 +57:16:48.8: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:51.42 +57:16:48.8: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 51.42 +57 16 48.8 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457992703739740416,2461199.8322,9.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457992703739740416 20260608.3322 9.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.71 02:35:42.02 +57:31:40.9
136.59089 -2.55232 galactic Per Second-epoch detections are separated by 1.2" and 8.6 pix
The object was found in VSX 2" Gaia DR3 458102998499428480
Type: VAR
# Max. Min./Amp. JD0 Period
12.230 G 12.260 G 0.062549500000 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:42.02 +57:31:40.9: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:42.02 +57:31:40.9: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 35 42.02 +57 31 40.9 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458102998499428480,2461199.8322,9.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458102998499428480 20260608.3322 9.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.56 02:31:56.68 +57:24:00.2
136.17362 -2.86481 galactic Per Second-epoch detections are separated by 0.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458017859371362944 | 02:31:56.62 +57:24:02.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.126+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:56.68 +57:24:00.2: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:56.68 +57:24:00.2: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 56.68 +57 24 00.2 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458017859371362944,2461199.8322,9.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458017859371362944 20260608.3322 9.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.76 02:38:19.87 +58:03:56.7
136.69993 -1.91977 galactic Cas Second-epoch detections are separated by 3.1" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458145368359426176 | 02:38:19.85 +58:03:55.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.841+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:19.87 +58:03:56.7: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:19.87 +58:03:56.7: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 38 19.87 +58 03 56.7 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458145368359426176,2461199.8322,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458145368359426176 20260608.3322 9.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.58 02:25:52.96 +56:47:30.0
135.63094 -3.73333 galactic Per Second-epoch detections are separated by 4.4" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457636397555905024 | 02:25:52.85 +56:47:29.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.107+/-0.035 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:52.96 +56:47:30.0: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:52.96 +56:47:30.0: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 52.96 +56 47 30.0 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457636397555905024,2461199.8322,9.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457636397555905024 20260608.3322 9.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.56 02:33:08.29 +57:28:10.5
136.29584 -2.73941 galactic Per Second-epoch detections are separated by 1.9" and 8.5 pix
The object was found in VSX 1" V0975 Per
Type: EB
# Max. Min./Amp. JD0 Period
11.890 V 11.990 V 2454774.38420 0.471920000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:08.29 +57:28:10.5: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:08.29 +57:28:10.5: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 08.29 +57 28 10.5 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0975 Per,2461199.8322,9.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0975 Per 20260608.3322 9.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.55 02:34:46.52 +57:13:22.5
136.59504 -2.88190 galactic Per Second-epoch detections are separated by 4.1" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457816167705315072 | 02:34:46.66 +57:13:24.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:46.52 +57:13:22.5: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:46.52 +57:13:22.5: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 46.52 +57 13 22.5 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457816167705315072,2461199.8322,9.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457816167705315072 20260608.3322 9.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.53 02:30:07.17 +56:30:20.8
136.27881 -3.78710 galactic Per Second-epoch detections are separated by 6.3" and 8.8 pix
The object was found in VSX 4" ASASSN-V J023007.46+563018.2
Type: L
# Max. Min./Amp. JD0 Period
12.620 V 12.910 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:07.17 +56:30:20.8: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:07.17 +56:30:20.8: 12.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 07.17 +56 30 20.8 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J023007.46+563018.2,2461199.8322,9.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J023007.46+563018.2 20260608.3322 9.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.69 02:29:48.78 +56:41:55.8
136.16766 -3.62355 galactic Per Second-epoch detections are separated by 2.5" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457599525253006080 | 02:29:48.84 +56:41:55.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.727+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:48.78 +56:41:55.8: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:48.78 +56:41:55.8: 12.40 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 48.78 +56 41 55.8 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457599525253006080,2461199.8322,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457599525253006080 20260608.3322 9.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.70 02:26:58.18 +56:22:12.1
135.92276 -4.07305 galactic Per Second-epoch detections are separated by 1.4" and 8.4 pix
The object was found in VSX24" Gaia DR3 457563348750748416
Type: ROT
# Max. Min./Amp. JD0 Period
16.950 G 17.010 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:58.18 +56:22:12.1: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:58.18 +56:22:12.1: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 58.18 +56 22 12.1 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457563348750748416,2461199.8322,9.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457563348750748416 20260608.3322 9.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.50 02:33:44.27 +56:59:34.7
136.55397 -3.14842 galactic Per Second-epoch detections are separated by 0.9" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457783766472214656 | 02:33:44.33 +56:59:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.389+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:44.27 +56:59:34.7: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:44.27 +56:59:34.7: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 44.27 +56 59 34.7 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457783766472214656,2461199.8322,9.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457783766472214656 20260608.3322 9.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.76 02:33:03.94 +57:33:09.8
136.25500 -2.66631 galactic Per Second-epoch detections are separated by 1.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.2769+57.5518 | 02:33:03.99 +57:33:10.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.000+/-0.039 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:03.94 +57:33:09.8: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:03.94 +57:33:09.8: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 03.94 +57 33 09.8 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.2769+57.5518,2461199.8322,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.2769+57.5518 20260608.3322 9.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.82 02:23:07.87 +56:29:01.2
135.38488 -4.15487 galactic Per Second-epoch detections are separated by 2.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.7790+56.4853 | 02:23:07.87 +56:29:01.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.176+/-0.037 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:07.87 +56:29:01.2: 12.68 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:07.87 +56:29:01.2: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 07.87 +56 29 01.2 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.7790+56.4853,2461199.8322,9.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.7790+56.4853 20260608.3322 9.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.62 02:25:56.53 +56:32:31.9
135.72795 -3.96340 galactic Per Second-epoch detections are separated by 1.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457615850432513152 | 02:25:56.55 +56:32:32.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.375+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:56.53 +56:32:31.9: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:56.53 +56:32:31.9: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 56.53 +56 32 31.9 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457615850432513152,2461199.8322,9.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457615850432513152 20260608.3322 9.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.78 02:35:58.93 +57:32:00.1
136.62363 -2.53259 galactic Per Second-epoch detections are separated by 3.6" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.9960+57.5329 | 02:35:59.06 +57:31:58.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.009+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:58.93 +57:32:00.1: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:58.93 +57:32:00.1: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 35 58.93 +57 32 00.1 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.9960+57.5329,2461199.8322,9.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.9960+57.5329 20260608.3322 9.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.69 02:27:44.66 +56:19:43.0
136.03809 -4.07274 galactic Per Second-epoch detections are separated by 0.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457559496157823232 | 02:27:44.64 +56:19:43.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.083+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:44.66 +56:19:43.0: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:44.66 +56:19:43.0: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 44.66 +56 19 43.0 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457559496157823232,2461199.8322,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457559496157823232 20260608.3322 9.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.87 02:25:56.42 +57:04:40.2
135.53586 -3.46324 galactic Per Second-epoch detections are separated by 1.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457667110856820608 | 02:25:52.98 +57:04:29.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.737+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:56.42 +57:04:40.2: 12.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:56.42 +57:04:40.2: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 56.42 +57 04 40.2 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457667110856820608,2461199.8322,9.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457667110856820608 20260608.3322 9.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.86 02:31:02.85 +57:42:08.9
135.94795 -2.63002 galactic Per Second-epoch detections are separated by 5.4" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458073659588630272 | 02:30:59.86 +57:42:44.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.009+/-0.051 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:02.85 +57:42:08.9: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:02.85 +57:42:08.9: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 02.85 +57 42 08.9 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458073659588630272,2461199.8322,9.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458073659588630272 20260608.3322 9.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.64 02:29:25.87 +55:58:55.7
136.38466 -4.30882 galactic Per Second-epoch detections are separated by 6.6" and 8.8 pix
The object was found in VSX 5" ASASSN-V J022926.29+555852.4
Type: SR
# Max. Min./Amp. JD0 Period
12.620 V 12.810 V 2457232.00000 79.400000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:25.87 +55:58:55.7: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:25.87 +55:58:55.7: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 25.87 +55 58 55.7 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J022926.29+555852.4,2461199.8322,9.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J022926.29+555852.4 20260608.3322 9.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.66 02:31:52.57 +56:53:49.0
136.35563 -3.33404 galactic Per Second-epoch detections are separated by 3.9" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.9796+56.9058 | 02:31:52.57 +56:53:48.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.336+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:52.57 +56:53:49.0: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:52.57 +56:53:49.0: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 52.57 +56 53 49.0 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.9796+56.9058,2461199.8322,9.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.9796+56.9058 20260608.3322 9.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.70 02:39:52.21 +58:24:37.9
136.74633 -1.52261 galactic Cas Second-epoch detections are separated by 8.6" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.9569+58.4206 | 02:39:52.01 +58:24:36.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.397+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:39:52.21 +58:24:37.9: 12.20 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:39:52.21 +58:24:37.9: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 39 52.21 +58 24 37.9 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.9569+58.4206,2461199.8322,9.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.9569+58.4206 20260608.3322 9.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.65 02:27:18.72 +56:15:53.5
136.00528 -4.15392 galactic Per Second-epoch detections are separated by 2.0" and 8.6 pix
The object was found in VSX23" Gaia DR3 457561768202818944
Type: ROT
# Max. Min./Amp. JD0 Period
17.200 G 17.310 G 3.692740000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:18.72 +56:15:53.5: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:18.72 +56:15:53.5: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 18.72 +56 15 53.5 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457561768202818944,2461199.8322,9.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457561768202818944 20260608.3322 9.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.87 02:36:25.89 +57:52:58.9
136.54126 -2.18749 galactic Cas Second-epoch detections are separated by 4.8" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458116884136450816 | 02:36:25.91 +57:52:57.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.972+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:25.89 +57:52:58.9: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:25.89 +57:52:58.9: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 36 25.89 +57 52 58.9 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458116884136450816,2461199.8322,9.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458116884136450816 20260608.3322 9.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.74 02:24:27.20 +56:50:28.9
135.43003 -3.75623 galactic Per Second-epoch detections are separated by 3.0" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458385130615759488 | 02:24:27.11 +56:50:29.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.330+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:27.20 +56:50:28.9: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:27.20 +56:50:28.9: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 27.20 +56 50 28.9 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458385130615759488,2461199.8322,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458385130615759488 20260608.3322 9.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.62 02:34:31.90 +56:11:08.8
136.96736 -3.85073 galactic Per Second-epoch detections are separated by 7.0" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.6110+56.1853 | 02:34:32.06 +56:11:11.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:31.90 +56:11:08.8: 11.40 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:31.90 +56:11:08.8: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 31.90 +56 11 08.8 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.6110+56.1853,2461199.8322,9.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.6110+56.1853 20260608.3322 9.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.85 02:27:31.55 +56:30:00.3
135.94737 -3.92398 galactic Per Second-epoch detections are separated by 2.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.8815+56.5001 | 02:27:31.56 +56:30:00.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.659+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:31.55 +56:30:00.3: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:31.55 +56:30:00.3: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 31.55 +56 30 00.3 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.8815+56.5001,2461199.8322,9.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.8815+56.5001 20260608.3322 9.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.71 02:25:53.52 +56:14:35.6
135.82861 -4.24510 galactic Per Second-epoch detections are separated by 3.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.4750+56.2475 | 02:25:53.37 +56:14:35.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.146+/-0.044 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:53.52 +56:14:35.6: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:53.52 +56:14:35.6: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 53.52 +56 14 35.6 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.4750+56.2475,2461199.8322,9.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.4750+56.2475 20260608.3322 9.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.64 02:30:58.33 +57:16:17.2
136.10042 -3.03338 galactic Per Second-epoch detections are separated by 2.8" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457992639322524672 | 02:30:58.40 +57:16:17.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.205+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:58.33 +57:16:17.2: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:58.33 +57:16:17.2: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 58.33 +57 16 17.2 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457992639322524672,2461199.8322,9.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457992639322524672 20260608.3322 9.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.96 02:22:27.17 +56:43:56.9
135.21073 -3.95378 galactic Per Second-epoch detections are separated by 7.9" and 9.5 pix
The object was found in VSX14" Gaia DR3 458293287035994112
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.980 G 13.020 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:27.17 +56:43:56.9: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:27.17 +56:43:56.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 27.17 +56 43 56.9 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458293287035994112,2461199.8322,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458293287035994112 20260608.3322 9.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.81 02:24:37.23 +56:45:53.9
135.47847 -3.81965 galactic Per Second-epoch detections are separated by 1.4" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.1592+56.7692 | 02:24:37.21 +56:45:54.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.502+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:37.23 +56:45:53.9: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:37.23 +56:45:53.9: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 37.23 +56 45 53.9 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.1592+56.7692,2461199.8322,9.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.1592+56.7692 20260608.3322 9.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.56 02:29:46.73 +56:03:52.6
136.39924 -4.21421 galactic Per Second-epoch detections are separated by 8.3" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457358564711288576 | 02:29:46.93 +56:03:52.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.336+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:46.73 +56:03:52.6: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:46.73 +56:03:52.6: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 46.73 +56 03 52.6 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457358564711288576,2461199.8322,9.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457358564711288576 20260608.3322 9.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.74 02:24:29.35 +56:34:20.6
135.52960 -4.00623 galactic Per Second-epoch detections are separated by 2.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457630006644514432 | 02:24:29.30 +56:34:20.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.688+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:29.35 +56:34:20.6: 11.40 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:29.35 +56:34:20.6: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 29.35 +56 34 20.6 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457630006644514432,2461199.8322,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457630006644514432 20260608.3322 9.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.76 02:31:18.77 +57:16:22.0
136.14265 -3.01485 galactic Per Second-epoch detections are separated by 3.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457993150416339840 | 02:31:18.94 +57:16:21.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.809+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:18.77 +57:16:22.0: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:18.77 +57:16:22.0: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 18.77 +57 16 22.0 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457993150416339840,2461199.8322,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457993150416339840 20260608.3322 9.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.72 02:31:20.63 +56:50:06.3
136.31154 -3.41878 galactic Per Second-epoch detections are separated by 4.3" and 9.1 pix
The object was found in VSX10" Gaia DR3 457965838726992640
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
17.280 G 17.380 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:20.63 +56:50:06.3: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:20.63 +56:50:06.3: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 20.63 +56 50 06.3 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457965838726992640,2461199.8322,9.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457965838726992640 20260608.3322 9.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.82 02:31:33.36 +57:25:43.5
136.11425 -2.85801 galactic Per Second-epoch detections are separated by 2.9" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458018542262985088 | 02:31:33.37 +57:25:44.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.136+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:33.36 +57:25:43.5: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:33.36 +57:25:43.5: 12.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 33.36 +57 25 43.5 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458018542262985088,2461199.8322,9.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458018542262985088 20260608.3322 9.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.79 02:21:07.65 +56:13:22.2
135.21353 -4.49526 galactic Per Second-epoch detections are separated by 4.7" and 8.8 pix
The object was found in VSX23" Gaia DR3 458255010286957952
Type: ROT
# Max. Min./Amp. JD0 Period
16.440 G 16.520 G 0.657900000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:07.65 +56:13:22.2: 12.27 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:07.65 +56:13:22.2: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 07.65 +56 13 22.2 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458255010286957952,2461199.8322,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458255010286957952 20260608.3322 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.68 02:30:09.68 +57:23:15.1
135.95535 -2.96657 galactic Per Second-epoch detections are separated by 1.9" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.5396+57.3872 | 02:30:09.52 +57:23:14.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.301+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:09.68 +57:23:15.1: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:09.68 +57:23:15.1: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 09.68 +57 23 15.1 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.5396+57.3872,2461199.8322,9.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.5396+57.3872 20260608.3322 9.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.62 02:33:18.10 +57:31:36.8
136.29419 -2.67806 galactic Per Second-epoch detections are separated by 4.2" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.3024+57.5280 | 02:33:17.98 +57:31:36.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.149+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:18.10 +57:31:36.8: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:18.10 +57:31:36.8: 11.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 18.10 +57 31 36.8 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.3024+57.5280,2461199.8322,9.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.3024+57.5280 20260608.3322 9.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.86 02:36:07.79 +57:32:58.9
136.63545 -2.50979 galactic Cas Second-epoch detections are separated by 4.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.0329+57.5501 | 02:36:07.91 +57:33:00.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.248+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:07.79 +57:32:58.9: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:07.79 +57:32:58.9: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 36 07.79 +57 32 58.9 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.0329+57.5501,2461199.8322,9.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.0329+57.5501 20260608.3322 9.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.72 02:34:41.26 +56:11:01.6
136.98819 -3.84415 galactic Per Second-epoch detections are separated by 7.5" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.6605+56.1803 | 02:34:41.56 +56:11:01.9 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:41.26 +56:11:01.6: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:41.26 +56:11:01.6: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 41.26 +56 11 01.6 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.6605+56.1803,2461199.8322,9.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.6605+56.1803 20260608.3322 9.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.04 02:26:20.11 +57:00:45.6
135.60947 -3.50486 galactic Per Second-epoch detections are separated by 1.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.5836+57.0007 | 02:26:20.11 +57:00:44.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.773+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:20.11 +57:00:45.6: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:20.11 +57:00:45.6: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 20.11 +57 00 45.6 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.5836+57.0007,2461199.8322,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.5836+57.0007 20260608.3322 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.76 02:30:53.15 +56:59:21.2
136.19551 -3.29941 galactic Per Second-epoch detections are separated by 2.7" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.7213+56.9885 | 02:30:53.11 +56:59:18.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.872+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:53.15 +56:59:21.2: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:53.15 +56:59:21.2: 12.52 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 53.15 +56 59 21.2 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.7213+56.9885,2461199.8322,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.7213+56.9885 20260608.3322 9.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.72 02:34:42.72 +57:17:58.8
136.55731 -2.81449 galactic Per Second-epoch detections are separated by 1.8" and 8.1 pix
The object was found in VSX19" Gaia DR3 458004424713842560
Type: ROT
# Max. Min./Amp. JD0 Period
17.430 G 17.480 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:42.72 +57:17:58.8: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:42.72 +57:17:58.8: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 42.72 +57 17 58.8 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458004424713842560,2461199.8322,9.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458004424713842560 20260608.3322 9.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.85 02:27:57.88 +56:22:23.8
136.05026 -4.02002 galactic Per Second-epoch detections are separated by 5.1" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457565543471774720 | 02:27:57.79 +56:22:24.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.062+/-0.034 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:57.88 +56:22:23.8: 12.53 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:57.88 +56:22:23.8: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 57.88 +56 22 23.8 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457565543471774720,2461199.8322,9.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457565543471774720 20260608.3322 9.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.86 02:33:08.50 +57:21:20.2
136.33993 -2.84453 galactic Per Second-epoch detections are separated by 0.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.2862+57.3553 | 02:33:08.69 +57:21:19.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.399+/-0.024 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:08.50 +57:21:20.2: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:08.50 +57:21:20.2: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 08.50 +57 21 20.2 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.2862+57.3553,2461199.8322,9.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.2862+57.3553 20260608.3322 9.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.76 02:37:52.11 +57:47:13.1
136.75508 -2.19986 galactic Cas Second-epoch detections are separated by 1.6" and 8.4 pix
The object was found in VSX 1" Gaia DR3 457947524984503552
Type: VAR
# Max. Min./Amp. JD0 Period
12.270 G 12.290 G 0.022696900000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:52.11 +57:47:13.1: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:52.11 +57:47:13.1: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 37 52.11 +57 47 13.1 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457947524984503552,2461199.8322,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457947524984503552 20260608.3322 9.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.82 02:25:45.87 +56:22:47.0
135.76316 -4.12392 galactic Per Second-epoch detections are separated by 1.4" and 8.0 pix
The object was found in VSX 3" Gaia DR3 457612448818505472
Type: ROT
# Max. Min./Amp. JD0 Period
12.560 G 12.600 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:45.87 +56:22:47.0: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:45.87 +56:22:47.0: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 45.87 +56 22 47.0 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457612448818505472,2461199.8322,9.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457612448818505472 20260608.3322 9.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.70 02:38:14.42 +57:58:50.6
136.72296 -2.00251 galactic Cas Second-epoch detections are separated by 1.4" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457956870833294720 | 02:38:14.37 +57:58:51.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.258+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:14.42 +57:58:50.6: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:14.42 +57:58:50.6: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 38 14.42 +57 58 50.6 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457956870833294720,2461199.8322,9.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457956870833294720 20260608.3322 9.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.80 02:33:33.71 +57:37:46.7
136.28698 -2.56979 galactic Per Second-epoch detections are separated by 4.2" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458025551649585024 | 02:33:33.59 +57:37:45.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.357+/-0.026 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:33.71 +57:37:46.7: 12.72 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:33.71 +57:37:46.7: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 33.71 +57 37 46.7 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458025551649585024,2461199.8322,9.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458025551649585024 20260608.3322 9.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.92 02:21:35.29 +56:14:56.5
135.26491 -4.44880 galactic Per Second-epoch detections are separated by 2.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.3836+56.2498 | 02:21:35.31 +56:14:55.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.767+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:35.29 +56:14:56.5: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:35.29 +56:14:56.5: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 35.29 +56 14 56.5 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.3836+56.2498,2461199.8322,9.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.3836+56.2498 20260608.3322 9.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.88 02:30:03.83 +56:36:39.2
136.23247 -3.69239 galactic Per Second-epoch detections are separated by 8.0" and 9.6 pix
The object was found in VSX13" Gaia DR3 457581456333710208
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.600 G 14.630 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:03.83 +56:36:39.2: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:03.83 +56:36:39.2: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 03.83 +56 36 39.2 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457581456333710208,2461199.8322,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457581456333710208 20260608.3322 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.76 02:26:36.42 +56:34:16.7
135.80319 -3.90337 galactic Per Second-epoch detections are separated by 0.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457621176191929088 | 02:26:36.32 +56:34:16.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.345+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:36.42 +56:34:16.7: 13.04 +/- 0.31 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:36.42 +56:34:16.7: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 36.42 +56 34 16.7 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457621176191929088,2461199.8322,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457621176191929088 20260608.3322 9.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.92 02:32:24.99 +57:27:18.3
136.21156 -2.78981 galactic Per Second-epoch detections are separated by 1.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.1070+57.4596 | 02:32:24.95 +57:27:18.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.867+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:24.99 +57:27:18.3: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:24.99 +57:27:18.3: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 24.99 +57 27 18.3 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.1070+57.4596,2461199.8322,9.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.1070+57.4596 20260608.3322 9.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.78 02:29:29.43 +57:10:39.0
135.94908 -3.19524 galactic Per Second-epoch detections are separated by 6.9" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.3768+57.1759 | 02:29:29.15 +57:10:37.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:29.43 +57:10:39.0: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:29.43 +57:10:39.0: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 29.43 +57 10 39.0 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.3768+57.1759,2461199.8322,9.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.3768+57.1759 20260608.3322 9.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.78 02:27:40.70 +56:20:28.5
136.02493 -4.06429 galactic Per Second-epoch detections are separated by 5.3" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:27:40.70 +56:20:28.5 (user input) | T | P | (position from user input) J-Ks=0.435+/-0.058 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:40.70 +56:20:28.5: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:40.70 +56:20:28.5: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 40.70 +56 20 28.5 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,9.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 9.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.89 02:34:04.61 +57:19:27.3
136.46862 -2.82501 galactic Per Second-epoch detections are separated by 0.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.5195+57.3241 | 02:34:04.70 +57:19:26.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.476+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:04.61 +57:19:27.3: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:04.61 +57:19:27.3: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 04.61 +57 19 27.3 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.5195+57.3241,2461199.8322,9.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.5195+57.3241 20260608.3322 9.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.75 02:26:10.21 +56:21:10.3
135.82539 -4.12891 galactic Per Second-epoch detections are separated by 2.7" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.5433+56.3532 | 02:26:10.21 +56:21:10.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.377+/-0.057 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:10.21 +56:21:10.3: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:10.21 +56:21:10.3: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 10.21 +56 21 10.3 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.5433+56.3532,2461199.8322,9.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.5433+56.3532 20260608.3322 9.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.94 02:22:29.14 +56:32:00.5
135.28383 -4.13899 galactic Per Second-epoch detections are separated by 4.4" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458283730723585024 | 02:22:29.08 +56:31:58.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.794+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:29.14 +56:32:00.5: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:29.14 +56:32:00.5: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 29.14 +56 32 00.5 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458283730723585024,2461199.8322,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458283730723585024 20260608.3322 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.89 02:34:35.60 +57:34:23.2
136.43641 -2.56864 galactic Per Second-epoch detections are separated by 1.6" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458106129538046976 | 02:34:35.65 +57:34:23.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.795+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:35.60 +57:34:23.2: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:35.60 +57:34:23.2: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 35.60 +57 34 23.2 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458106129538046976,2461199.8322,9.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458106129538046976 20260608.3322 9.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.77 02:34:46.10 +57:12:52.3
136.59743 -2.89000 galactic Per Second-epoch detections are separated by 0.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457816167705315072 | 02:34:46.66 +57:13:24.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:46.10 +57:12:52.3: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:46.10 +57:12:52.3: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 46.10 +57 12 52.3 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457816167705315072,2461199.8322,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457816167705315072 20260608.3322 9.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.87 02:34:38.93 +57:26:15.3
136.49589 -2.69068 galactic Per Second-epoch detections are separated by 2.1" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458007585809735808 | 02:34:38.99 +57:26:17.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.174+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:38.93 +57:26:15.3: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:38.93 +57:26:15.3: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 38.93 +57 26 15.3 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458007585809735808,2461199.8322,9.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458007585809735808 20260608.3322 9.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.83 02:32:54.63 +57:10:57.1
136.37725 -3.01642 galactic Per Second-epoch detections are separated by 1.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458000507703592576 | 02:32:54.74 +57:10:58.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.249+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:54.63 +57:10:57.1: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:54.63 +57:10:57.1: 12.52 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 54.63 +57 10 57.1 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458000507703592576,2461199.8322,9.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458000507703592576 20260608.3322 9.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.82 02:22:37.79 +56:37:17.0
135.27205 -4.04963 galactic Per Second-epoch detections are separated by 2.5" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458290469537534208 | 02:22:37.88 +56:37:18.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.731+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:37.79 +56:37:17.0: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:37.79 +56:37:17.0: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 37.79 +56 37 17.0 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458290469537534208,2461199.8322,9.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458290469537534208 20260608.3322 9.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.04 02:23:18.87 +57:06:02.1
135.19344 -3.56773 galactic Per Second-epoch detections are separated by 0.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:23:18.87 +57:06:02.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:18.87 +57:06:02.1: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:18.87 +57:06:02.1: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 18.87 +57 06 02.1 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.93 02:24:23.45 +56:13:56.3
135.63695 -4.32931 galactic Per Second-epoch detections are separated by 2.1" and 8.5 pix
The object was found in VSX 5" Gaia DR3 457511117649033728
Type: E
# Max. Min./Amp. JD0 Period
16.730 G 16.910 G 3.014200000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:23.45 +56:13:56.3: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:23.45 +56:13:56.3: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 23.45 +56 13 56.3 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457511117649033728,2461199.8322,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457511117649033728 20260608.3322 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.89 02:20:23.58 +56:22:39.7
135.06472 -4.38414 galactic Per Second-epoch detections are separated by 5.1" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458269338297619840 | 02:20:23.69 +56:22:37.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:23.58 +56:22:39.7: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:23.58 +56:22:39.7: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 20 23.58 +56 22 39.7 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458269338297619840,2461199.8322,9.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458269338297619840 20260608.3322 9.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.77 02:26:45.86 +56:23:26.2
135.88874 -4.06411 galactic Per Second-epoch detections are separated by 2.5" and 7.9 pix
The object was found in VSX 1" Gaia DR3 457610245491390464
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.280 G 12.300 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:45.86 +56:23:26.2: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:45.86 +56:23:26.2: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 45.86 +56 23 26.2 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457610245491390464,2461199.8322,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457610245491390464 20260608.3322 9.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.89 02:30:55.12 +57:08:07.5
136.14477 -3.16220 galactic Per Second-epoch detections are separated by 2.4" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457984977100976256 | 02:30:55.00 +57:08:08.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.397+/-0.029 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:55.12 +57:08:07.5: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:55.12 +57:08:07.5: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 55.12 +57 08 07.5 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457984977100976256,2461199.8322,9.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457984977100976256 20260608.3322 9.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.77 02:32:06.03 +57:05:00.6
136.31320 -3.14980 galactic Per Second-epoch detections are separated by 5.1" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457975115856080512 | 02:32:05.87 +57:04:58.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.175+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:06.03 +57:05:00.6: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:06.03 +57:05:00.6: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 06.03 +57 05 00.6 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457975115856080512,2461199.8322,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457975115856080512 20260608.3322 9.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.90 02:25:39.55 +56:48:00.4
135.59928 -3.73636 galactic Per Second-epoch detections are separated by 1.4" and 8.5 pix
The object was found in VSX19" Gaia DR3 457639318133538560
Type: ROT
# Max. Min./Amp. JD0 Period
14.980 G 15.010 G 7.447400000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:39.55 +56:48:00.4: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:39.55 +56:48:00.4: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 39.55 +56 48 00.4 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457639318133538560,2461199.8322,9.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457639318133538560 20260608.3322 9.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.92 02:22:51.67 +56:24:33.0
135.37573 -4.23769 galactic Per Second-epoch detections are separated by 1.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458278890305908352 | 02:22:51.69 +56:24:32.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.372+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:51.67 +56:24:33.0: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:51.67 +56:24:33.0: 12.52 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 51.67 +56 24 33.0 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458278890305908352,2461199.8322,9.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458278890305908352 20260608.3322 9.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.93 02:25:12.20 +56:44:30.7
135.56155 -3.81301 galactic Per Second-epoch detections are separated by 0.9" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457632888558943232 | 02:25:12.18 +56:44:30.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.121+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:12.20 +56:44:30.7: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:12.20 +56:44:30.7: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 12.20 +56 44 30.7 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457632888558943232,2461199.8322,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457632888558943232 20260608.3322 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.96 02:25:05.47 +56:20:33.3
135.68903 -4.19180 galactic Per Second-epoch detections are separated by 0.6" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.2664+56.3410 | 02:25:05.54 +56:20:34.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.752+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:05.47 +56:20:33.3: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:05.47 +56:20:33.3: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 05.47 +56 20 33.3 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.2664+56.3410,2461199.8322,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.2664+56.3410 20260608.3322 9.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.78 02:25:48.30 +56:35:16.7
135.69387 -3.92740 galactic Per Second-epoch detections are separated by 5.2" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457616155366363520 | 02:25:48.08 +56:35:15.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.147+/-0.038 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:48.30 +56:35:16.7: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:48.30 +56:35:16.7: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 48.30 +56 35 16.7 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457616155366363520,2461199.8322,9.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457616155366363520 20260608.3322 9.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.96 02:25:01.82 +56:15:07.5
135.71329 -4.27942 galactic Per Second-epoch detections are separated by 3.1" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457516413349915264 | 02:25:01.66 +56:15:05.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:01.82 +56:15:07.5: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:01.82 +56:15:07.5: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 01.82 +56 15 07.5 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457516413349915264,2461199.8322,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457516413349915264 20260608.3322 9.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.78 02:32:01.41 +55:53:20.2
136.75718 -4.25921 galactic Per Second-epoch detections are separated by 5.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457339185819254144 | 02:32:01.84 +55:53:19.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:01.41 +55:53:20.2: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:01.41 +55:53:20.2: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 01.41 +55 53 20.2 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457339185819254144,2461199.8322,9.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457339185819254144 20260608.3322 9.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.88 02:35:41.37 +57:27:01.8
136.61993 -2.62424 galactic Per Second-epoch detections are separated by 2.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458101078656993664 | 02:35:41.28 +57:27:02.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.265+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:41.37 +57:27:01.8: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:41.37 +57:27:01.8: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 35 41.37 +57 27 01.8 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458101078656993664,2461199.8322,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458101078656993664 20260608.3322 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.95 02:24:54.82 +56:45:04.1
135.52104 -3.81840 galactic Per Second-epoch detections are separated by 3.1" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.2248+56.7481 | 02:24:54.80 +56:45:03.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.759+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:54.82 +56:45:04.1: 11.27 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:54.82 +56:45:04.1: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 54.82 +56 45 04.1 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.2248+56.7481,2461199.8322,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.2248+56.7481 20260608.3322 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.04 02:23:46.82 +57:05:04.4
135.25845 -3.56068 galactic Per Second-epoch detections are separated by 5.1" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.9449+57.0839 | 02:23:46.82 +57:05:04.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.365+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:46.82 +57:05:04.4: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:46.82 +57:05:04.4: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 46.82 +57 05 04.4 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.9449+57.0839,2461199.8322,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.9449+57.0839 20260608.3322 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.95 02:27:24.28 +56:17:59.4
136.00458 -4.11666 galactic Per Second-epoch detections are separated by 1.0" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.8584+56.2997 | 02:27:24.37 +56:17:58.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.040+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:24.28 +56:17:59.4: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:24.28 +56:17:59.4: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 24.28 +56 17 59.4 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.8584+56.2997,2461199.8322,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.8584+56.2997 20260608.3322 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.94 02:23:29.57 +56:10:15.1
135.54125 -4.43063 galactic Per Second-epoch detections are separated by 4.5" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.8681+56.1720 | 02:23:29.47 +56:10:13.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.411+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:29.57 +56:10:15.1: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:29.57 +56:10:15.1: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 29.57 +56 10 15.1 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.8681+56.1720,2461199.8322,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.8681+56.1720 20260608.3322 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.84 02:34:46.00 +58:00:26.7
136.28914 -2.15937 galactic Per Second-epoch detections are separated by 2.5" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458132376076756736 | 02:34:46.21 +58:00:26.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.245+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:46.00 +58:00:26.7: 12.81 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:46.00 +58:00:26.7: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 46.00 +58 00 26.7 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458132376076756736,2461199.8322,9.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458132376076756736 20260608.3322 9.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.88 02:32:58.19 +57:38:43.0
136.20773 -2.58568 galactic Per Second-epoch detections are separated by 2.3" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.2415+57.6480 | 02:32:58.09 +57:38:42.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.151+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:58.19 +57:38:43.0: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:58.19 +57:38:43.0: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 58.19 +57 38 43.0 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.2415+57.6480,2461199.8322,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.2415+57.6480 20260608.3322 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.88 02:37:47.78 +57:52:43.0
136.70970 -2.11966 galactic Cas Second-epoch detections are separated by 2.7" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.4491+57.8783 | 02:37:47.80 +57:52:42.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.359+/-0.040 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:47.78 +57:52:43.0: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:47.78 +57:52:43.0: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 37 47.78 +57 52 43.0 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.4491+57.8783,2461199.8322,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.4491+57.8783 20260608.3322 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.04 02:24:54.07 +56:55:39.8
135.45684 -3.65384 galactic Per Second-epoch detections are separated by 3.4" and 7.5 pix
The object was found in VSX 3" Gaia DR3 458391658965964672
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.430 G 12.470 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:54.07 +56:55:39.8: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:54.07 +56:55:39.8: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 54.07 +56 55 39.8 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458391658965964672,2461199.8322,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458391658965964672 20260608.3322 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.86 02:37:58.92 +58:07:38.9
136.63293 -1.88164 galactic Cas Second-epoch detections are separated by 2.0" and 8.5 pix
The object was found in VSX 3" Gaia DR3 458146639669716992
Type: L
# Max. Min./Amp. JD0 Period
11.580 G 11.700 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:58.92 +58:07:38.9: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:58.92 +58:07:38.9: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 37 58.92 +58 07 38.9 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458146639669716992,2461199.8322,9.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458146639669716992 20260608.3322 9.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.20 02:27:22.03 +56:50:16.1
135.80422 -3.61718 galactic Per Second-epoch detections are separated by 2.4" and 7.8 pix
The object was found in VSX 2" Gaia DR3 457648423465255040
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.720 G 12.790 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:22.03 +56:50:16.1: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:22.03 +56:50:16.1: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 22.03 +56 50 16.1 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457648423465255040,2461199.8322,10.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457648423465255040 20260608.3322 10.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.09 02:36:17.73 +57:48:52.1
136.55163 -2.25763 galactic Cas Second-epoch detections are separated by 2.3" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.0727+57.8140 | 02:36:17.73 +57:48:52.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:17.73 +57:48:52.1: 11.89 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:17.73 +57:48:52.1: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 36 17.73 +57 48 52.1 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.0727+57.8140,2461199.8322,10.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.0727+57.8140 20260608.3322 10.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.06 02:25:54.98 +56:55:26.7
135.58785 -3.60800 galactic Per Second-epoch detections are separated by 6.3" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457641792034790272 | 02:25:54.85 +56:55:25.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.390+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:54.98 +56:55:26.7: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:54.98 +56:55:26.7: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 54.98 +56 55 26.7 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457641792034790272,2461199.8322,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457641792034790272 20260608.3322 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.00 02:27:32.20 +57:08:35.3
135.71483 -3.32427 galactic Per Second-epoch detections are separated by 1.1" and 8.3 pix
The object was found in VSX12" ZTF J022730.95+570829.5
Type: RS
# Max. Min./Amp. JD0 Period
16.665 g Y 0.087 g 2458464.76450 0.560941800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:32.20 +57:08:35.3: 11.73 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:32.20 +57:08:35.3: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 32.20 +57 08 35.3 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J022730.95+570829.5,2461199.8322,10.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J022730.95+570829.5 20260608.3322 10.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.07 02:20:13.03 +56:15:34.8
135.08166 -4.50347 galactic Per Second-epoch detections are separated by 1.9" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.0557+56.2668 | 02:20:13.25 +56:15:33.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:13.03 +56:15:34.8: 10.51 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:13.03 +56:15:34.8: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 20 13.03 +56 15 34.8 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.0557+56.2668,2461199.8322,10.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.0557+56.2668 20260608.3322 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.18 02:22:27.81 +56:33:28.7
135.27247 -4.11705 galactic Per Second-epoch detections are separated by 0.8" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:22:27.81 +56:33:28.7 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.668+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:27.81 +56:33:28.7: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:27.81 +56:33:28.7: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 27.81 +56 33 28.7 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.19 02:27:58.93 +57:31:01.3
135.63473 -2.95412 galactic Per Second-epoch detections are separated by 3.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:27:58.93 +57:31:01.3 (user input) | T | P | (position from user input) J-Ks=0.247+/-0.042 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:58.93 +57:31:01.3: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:58.93 +57:31:01.3: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 58.93 +57 31 01.3 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.95 02:33:32.05 +57:51:40.8
136.19454 -2.35727 galactic Per Second-epoch detections are separated by 4.0" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458124683796663808 | 02:33:32.09 +57:51:40.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.260+/-0.026 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:32.05 +57:51:40.8: 11.77 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:32.05 +57:51:40.8: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 32.05 +57 51 40.8 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458124683796663808,2461199.8322,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458124683796663808 20260608.3322 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.93 02:34:38.40 +57:44:07.3
136.37922 -2.41666 galactic Per Second-epoch detections are separated by 6.5" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:34:38.40 +57:44:07.3 (user input) | T | P | (position from user input) J-Ks=0.424+/-0.029 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:38.40 +57:44:07.3: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:38.40 +57:44:07.3: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 38.40 +57 44 07.3 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.94 02:25:47.88 +56:43:23.2
135.64461 -3.80150 galactic Per Second-epoch detections are separated by 2.4" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.4463+56.7250 | 02:25:47.88 +56:43:23.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.107+/-0.035 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:47.88 +56:43:23.2: 12.75 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:47.88 +56:43:23.2: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 47.88 +56 43 23.2 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.4463+56.7250,2461199.8322,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.4463+56.7250 20260608.3322 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.90 02:30:08.47 +57:20:50.2
135.96782 -3.00495 galactic Per Second-epoch detections are separated by 5.9" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.5339+57.3465 | 02:30:08.14 +57:20:47.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:08.47 +57:20:50.2: 12.64 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:08.47 +57:20:50.2: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 08.47 +57 20 50.2 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.5339+57.3465,2461199.8322,9.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.5339+57.3465 20260608.3322 9.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.06 02:38:25.27 +58:17:31.8
136.62006 -1.70756 galactic Cas Second-epoch detections are separated by 2.6" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 464156737721642880 | 02:38:25.23 +58:17:29.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.419+/-0.038 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:25.27 +58:17:31.8: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:25.27 +58:17:31.8: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 38 25.27 +58 17 31.8 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 464156737721642880,2461199.8322,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 464156737721642880 20260608.3322 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.95 02:38:01.91 +58:25:43.4
136.51860 -1.60283 galactic Cas Second-epoch detections are separated by 5.9" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 464170447257250176 | 02:38:01.87 +58:25:42.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.360+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:01.91 +58:25:43.4: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:01.91 +58:25:43.4: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 38 01.91 +58 25 43.4 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 464170447257250176,2461199.8322,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 464170447257250176 20260608.3322 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.06 02:22:07.92 +56:28:58.2
135.25540 -4.20334 galactic Per Second-epoch detections are separated by 3.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.5225+56.4733 | 02:22:07.85 +56:28:58.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.780+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:07.92 +56:28:58.2: 10.29 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:07.92 +56:28:58.2: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 07.92 +56 28 58.2 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.5225+56.4733,2461199.8322,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.5225+56.4733 20260608.3322 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.85 02:34:18.98 +56:07:35.1
136.96272 -3.91707 galactic Per Second-epoch detections are separated by 5.9" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.5805+56.1272 | 02:34:19.32 +56:07:38.2 (Gaia DR3) | SINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:18.98 +56:07:35.1: 12.52 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:18.98 +56:07:35.1: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 18.98 +56 07 35.1 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.5805+56.1272,2461199.8322,9.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.5805+56.1272 20260608.3322 9.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.23 02:27:20.09 +56:49:46.3
135.80310 -3.62650 galactic Per Second-epoch detections are separated by 5.1" and 9.0 pix
The object was found in VSX20" Gaia DR3 457648801422382592
Type: RS
# Max. Min./Amp. JD0 Period
16.370 G 16.450 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:20.09 +56:49:46.3: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:20.09 +56:49:46.3: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 20.09 +56 49 46.3 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457648801422382592,2461199.8322,10.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457648801422382592 20260608.3322 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.14 02:28:36.20 +56:28:40.0
136.09431 -3.89046 galactic Per Second-epoch detections are separated by 3.0" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457567884236316928 | 02:28:36.25 +56:28:37.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.955+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:36.20 +56:28:40.0: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:36.20 +56:28:40.0: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 28 36.20 +56 28 40.0 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457567884236316928,2461199.8322,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457567884236316928 20260608.3322 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.07 02:23:45.93 +56:58:54.6
135.29254 -3.65763 galactic Per Second-epoch detections are separated by 0.6" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.9414+56.9816 | 02:23:45.95 +56:58:54.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.342+/-0.035 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:45.93 +56:58:54.6: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:45.93 +56:58:54.6: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 45.93 +56 58 54.6 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.9414+56.9816,2461199.8322,10.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.9414+56.9816 20260608.3322 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.11 02:28:30.00 +56:31:48.6
136.06176 -3.84695 galactic Per Second-epoch detections are separated by 2.0" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:28:30.00 +56:31:48.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:30.00 +56:31:48.6: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:30.00 +56:31:48.6: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 28 30.00 +56 31 48.6 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.14 02:28:30.82 +57:06:37.8
135.85040 -3.30631 galactic Per Second-epoch detections are separated by 4.7" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:28:30.82 +57:06:37.8 (user input) | T | P | (position from user input) J-Ks=0.018+/-0.038 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:30.82 +57:06:37.8: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:30.82 +57:06:37.8: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 28 30.82 +57 06 37.8 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.07 02:25:01.45 +56:33:15.8
135.60509 -3.99703 galactic Per Second-epoch detections are separated by 1.5" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457627257865445376 | 02:25:01.50 +56:33:18.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:01.45 +56:33:15.8: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:01.45 +56:33:15.8: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 01.45 +56 33 15.8 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457627257865445376,2461199.8322,10.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457627257865445376 20260608.3322 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.04 02:30:19.39 +57:30:27.0
135.93085 -2.84712 galactic Per Second-epoch detections are separated by 2.7" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458046476730269440 | 02:30:19.51 +57:30:27.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.239+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:19.39 +57:30:27.0: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:19.39 +57:30:27.0: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 30 19.39 +57 30 27.0 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458046476730269440,2461199.8322,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458046476730269440 20260608.3322 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.20 02:33:38.71 +57:12:31.9
136.45919 -2.95397 galactic Per Second-epoch detections are separated by 0.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:33:38.71 +57:12:31.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:38.71 +57:12:31.9: 12.40 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:38.71 +57:12:31.9: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 38.71 +57 12 31.9 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.21 02:32:02.17 +57:26:35.5
136.16868 -2.82022 galactic Per Second-epoch detections are separated by 2.6" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.0091+57.4427 | 02:32:02.20 +57:26:33.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.392+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:02.17 +57:26:35.5: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:02.17 +57:26:35.5: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 02.17 +57 26 35.5 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.0091+57.4427,2461199.8322,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.0091+57.4427 20260608.3322 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.98 02:33:09.48 +57:50:43.7
136.15436 -2.39109 galactic Per Second-epoch detections are separated by 8.3" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.2794+57.8463 | 02:33:09.37 +57:50:41.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.219+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:09.48 +57:50:43.7: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:09.48 +57:50:43.7: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 09.48 +57 50 43.7 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.2794+57.8463,2461199.8322,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.2794+57.8463 20260608.3322 9.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.96 02:24:54.81 +56:34:32.0
135.58329 -3.98263 galactic Per Second-epoch detections are separated by 2.6" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457627459720286848 | 02:24:54.75 +56:34:32.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.681+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:54.81 +56:34:32.0: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:54.81 +56:34:32.0: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 54.81 +56 34 32.0 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457627459720286848,2461199.8322,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457627459720286848 20260608.3322 9.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.30 02:24:12.77 +56:08:04.7
135.64817 -4.42944 galactic Per Second-epoch detections are separated by 7.0" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:24:12.77 +56:08:04.7 (user input) | T | P | (position from user input) J-Ks=0.423+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:12.77 +56:08:04.7: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:12.77 +56:08:04.7: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 12.77 +56 08 04.7 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.14 02:24:25.62 +56:20:53.3
135.60075 -4.21913 galactic Per Second-epoch detections are separated by 5.6" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:24:25.62 +56:20:53.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:25.62 +56:20:53.3: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:25.62 +56:20:53.3: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 25.62 +56 20 53.3 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.12 02:31:40.18 +57:12:25.9
136.21217 -3.05740 galactic Per Second-epoch detections are separated by 5.4" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.9315+57.2038 | 02:31:40.17 +57:12:25.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.768+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:40.18 +57:12:25.9: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:40.18 +57:12:25.9: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 40.18 +57 12 25.9 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.9315+57.2038,2461199.8322,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.9315+57.2038 20260608.3322 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.42 02:21:22.21 +56:42:51.2
135.07717 -4.02188 galactic Per Second-epoch detections are separated by 2.0" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.3423+56.7145 | 02:21:22.21 +56:42:51.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.473+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:22.21 +56:42:51.2: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:22.21 +56:42:51.2: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 22.21 +56 42 51.2 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.3423+56.7145,2461199.8322,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.3423+56.7145 20260608.3322 10.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.06 02:32:03.60 +57:19:01.2
136.21952 -2.93579 galactic Per Second-epoch detections are separated by 3.7" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458014045440456832 | 02:32:03.54 +57:19:01.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.463+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:03.60 +57:19:01.2: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:03.60 +57:19:01.2: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 03.60 +57 19 01.2 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458014045440456832,2461199.8322,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458014045440456832 20260608.3322 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.16 02:29:35.90 +56:47:29.8
136.10581 -3.54830 galactic Per Second-epoch detections are separated by 2.9" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457604099401132544 | 02:29:35.73 +56:47:29.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.192+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:35.90 +56:47:29.8: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:35.90 +56:47:29.8: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 35.90 +56 47 29.8 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457604099401132544,2461199.8322,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457604099401132544 20260608.3322 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.81 00:45:31.36 +61:20:32.6
122.22253 -1.52121 galactic Cas Second-epoch detections are separated by 0.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:45:31.36 +61:20:32.6 (user input) | T | P | (position from user input) J-Ks=0.419+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:45:31.36 +61:20:32.6: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:45:31.36 +61:20:32.6: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 00 45 31.36 +61 20 32.6 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.28 02:24:19.17 +56:16:19.6
135.61360 -4.29554 galactic Per Second-epoch detections are separated by 3.0" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.0830+56.2756 | 02:24:19.17 +56:16:19.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.353+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:19.17 +56:16:19.6: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:19.17 +56:16:19.6: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 19.17 +56 16 19.6 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.0830+56.2756,2461199.8322,10.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.0830+56.2756 20260608.3322 10.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.23 02:21:10.37 +56:34:16.2
135.10049 -4.16561 galactic Per Second-epoch detections are separated by 0.9" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.2899+56.5668 | 02:21:10.37 +56:34:16.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.815+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:10.37 +56:34:16.2: 12.65 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:10.37 +56:34:16.2: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 10.37 +56 34 16.2 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.2899+56.5668,2461199.8322,10.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.2899+56.5668 20260608.3322 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.34 02:25:03.41 +56:05:16.2
135.77514 -4.43169 galactic Per Second-epoch detections are separated by 2.1" and 8.0 pix
The object was found in VSX 4" ASASSN-V J022503.49+560512.5
Type: SR
# Max. Min./Amp. JD0 Period
14.110 V 14.890 V 2458345.86760 61.251834500000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:03.41 +56:05:16.2: 10.71 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:03.41 +56:05:16.2: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 03.41 +56 05 16.2 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J022503.49+560512.5,2461199.8322,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J022503.49+560512.5 20260608.3322 10.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.24 02:31:07.14 +56:54:53.9
136.25293 -3.35630 galactic Per Second-epoch detections are separated by 2.7" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457978066491205248 | 02:31:07.21 +56:54:51.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.801+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:07.14 +56:54:53.9: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:07.14 +56:54:53.9: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 07.14 +56 54 53.9 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457978066491205248,2461199.8322,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457978066491205248 20260608.3322 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.38 02:29:01.50 +57:51:35.8
135.63884 -2.58399 galactic Per Second-epoch detections are separated by 5.9" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:29:01.50 +57:51:35.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:01.50 +57:51:35.8: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:01.50 +57:51:35.8: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 01.50 +57 51 35.8 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.39 02:35:08.92 +57:20:11.7
136.59731 -2.75756 galactic Per Second-epoch detections are separated by 7.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.7924+57.3397 | 02:35:08.92 +57:20:11.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:08.92 +57:20:11.7: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:08.92 +57:20:11.7: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 35 08.92 +57 20 11.7 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.7924+57.3397,2461199.8322,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.7924+57.3397 20260608.3322 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.23 02:38:11.28 +57:54:13.4
136.74741 -2.07585 galactic Cas Second-epoch detections are separated by 5.6" and 9.3 pix
The object was found in VSX 2" Gaia DR3 457950548641449088
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.500 G 13.540 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:11.28 +57:54:13.4: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:11.28 +57:54:13.4: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 38 11.28 +57 54 13.4 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457950548641449088,2461199.8322,10.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457950548641449088 20260608.3322 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.28 02:28:13.34 +57:23:00.9
135.71361 -3.06657 galactic Per Second-epoch detections are separated by 3.6" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.0558+57.3730 | 02:28:13.34 +57:23:00.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.344+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:13.34 +57:23:00.9: 12.38 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:13.34 +57:23:00.9: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 28 13.34 +57 23 00.9 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.0558+57.3730,2461199.8322,10.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.0558+57.3730 20260608.3322 10.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.92 01:31:48.44 +64:21:56.3
127.28200 1.83539 galactic Cas Second-epoch detections are separated by 2.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:31:48.44 +64:21:56.3 (user input) | T | P | (position from user input) J-Ks=0.974+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.44 +64:21:56.3: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.44 +64:21:56.3: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 31 48.44 +64 21 56.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.79 01:19:41.78 +62:51:03.2
126.14909 0.15579 galactic Cas Second-epoch detections are separated by 1.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:19:41.78 +62:51:03.2 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:41.78 +62:51:03.2: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:41.78 +62:51:03.2: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 19 41.78 +62 51 03.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.40 02:37:45.34 +58:30:48.3
136.45169 -1.53957 galactic Cas Second-epoch detections are separated by 3.7" and 8.4 pix
The object was found in VSX 5" ASASSN-V J023745.82+583044.7
Type: SR
# Max. Min./Amp. JD0 Period
14.930 V 15.490 V 2457362.90000 66.700000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:45.34 +58:30:48.3: 13.12 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:45.34 +58:30:48.3: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 37 45.34 +58 30 48.3 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J023745.82+583044.7,2461199.8322,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J023745.82+583044.7 20260608.3322 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.51 02:35:39.23 +57:45:01.8
136.49802 -2.35003 galactic Cas Second-epoch detections are separated by 2.2" and 8.5 pix
The object was found in VSX 2" ASASSN-V J023539.35+574500.1
Type: SR
# Max. Min./Amp. JD0 Period
15.620 g Y 0.380 g 2459078.94400 37.690000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:39.23 +57:45:01.8: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:39.23 +57:45:01.8: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 35 39.23 +57 45 01.8 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J023539.35+574500.1,2461199.8322,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J023539.35+574500.1 20260608.3322 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.76 01:38:33.81 +60:47:25.6
128.65248 -1.55681 galactic Cas Second-epoch detections are separated by 4.9" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:38:33.81 +60:47:25.6 (user input) | T | P | (position from user input) J-Ks=0.216+/-0.037 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:33.81 +60:47:25.6: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:33.81 +60:47:25.6: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 38 33.81 +60 47 25.6 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.55 02:35:28.55 +57:41:15.0
136.50077 -2.41731 galactic Cas Second-epoch detections are separated by 4.2" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.8701+57.6882 | 02:35:28.55 +57:41:15.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:28.55 +57:41:15.0: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:28.55 +57:41:15.0: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 35 28.55 +57 41 15.0 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.8701+57.6882,2461199.8322,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.8701+57.6882 20260608.3322 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.44 02:24:51.53 +56:15:26.9
135.68904 -4.28281 galactic Per Second-epoch detections are separated by 3.5" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457516855722787712 | 02:24:51.55 +56:15:25.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.076+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:51.53 +56:15:26.9: 11.76 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:51.53 +56:15:26.9: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 24 51.53 +56 15 26.9 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457516855722787712,2461199.8322,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457516855722787712 20260608.3322 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.24 02:26:24.74 +56:14:06.4
135.89920 -4.22676 galactic Per Second-epoch detections are separated by 3.2" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.6025+56.2349 | 02:26:24.62 +56:14:05.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.297+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:24.74 +56:14:06.4: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:24.74 +56:14:06.4: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 26 24.74 +56 14 06.4 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.6025+56.2349,2461199.8322,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.6025+56.2349 20260608.3322 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.60 02:19:14.48 +56:36:18.0
134.83805 -4.22338 galactic Per Second-epoch detections are separated by 5.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:19:14.48 +56:36:18.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:14.48 +56:36:18.0: 12.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:14.48 +56:36:18.0: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 19 14.48 +56 36 18.0 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 11.09 01:31:48.60 +64:22:28.2
127.28090 1.84419 galactic Cas Second-epoch detections are separated by 2.7" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:31:48.60 +64:22:28.2 (user input) | T | P | (position from user input) J-Ks=0.844+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.60 +64:22:28.2: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.60 +64:22:28.2: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 31 48.60 +64 22 28.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.95 02:32:01.89 +57:03:30.5
136.31401 -3.17652 galactic Per Second-epoch detections are separated by 1.3" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.9985+57.0505 | 02:32:01.89 +57:03:30.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.309+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:01.89 +57:03:30.5: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:01.89 +57:03:30.5: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 01.89 +57 03 30.5 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.9985+57.0505,2461199.8322,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.9985+57.0505 20260608.3322 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.61 02:32:59.26 +57:53:54.0
136.11320 -2.35090 galactic Per Second-epoch detections are separated by 1.4" and 8.6 pix
The object was found in VSX 1" Gaia DR3 458172615631671808
Type: VAR
# Max. Min./Amp. JD0 Period
12.120 G 12.150 G 0.251708000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:59.26 +57:53:54.0: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:59.26 +57:53:54.0: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 59.26 +57 53 54.0 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458172615631671808,2461199.8322,9.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458172615631671808 20260608.3322 9.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.29 02:38:06.09 +59:06:42.5
136.25399 -0.97299 galactic Cas Second-epoch detections are separated by 5.1" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:38:06.09 +59:06:42.5 (user input) | T | P | (position from user input) J-Ks=0.360+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:06.09 +59:06:42.5: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:06.09 +59:06:42.5: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 38 06.09 +59 06 42.5 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.19 02:15:35.85 +56:21:36.3
134.44162 -4.61936 galactic Per Second-epoch detections are separated by 0.2" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J033.8885+56.3660 | 02:15:35.87 +56:21:38.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.581+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:35.85 +56:21:36.3: 12.91 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:35.85 +56:21:36.3: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 15 35.85 +56 21 36.3 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J033.8885+56.3660,2461199.8322,9.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J033.8885+56.3660 20260608.3322 9.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.74 02:38:02.06 +58:50:39.8
136.35287 -1.22161 galactic Cas Second-epoch detections are separated by 1.9" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.5186+58.8445 | 02:38:02.39 +58:50:41.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:02.06 +58:50:39.8: 10.12 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:02.06 +58:50:39.8: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 38 02.06 +58 50 39.8 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.5186+58.8445,2461199.8322,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.5186+58.8445 20260608.3322 9.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.32 02:25:13.30 +56:30:31.2
135.64687 -4.03012 galactic Per Second-epoch detections are separated by 0.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.2868+56.5107 | 02:25:13.36 +56:30:32.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.108+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:13.30 +56:30:31.2: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:13.30 +56:30:31.2: 10.83 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 13.30 +56 30 31.2 8.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J036.2868+56.5107,2461199.8322,8.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J036.2868+56.5107 20260608.3322 8.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.18 02:05:05.77 +58:16:23.4
132.50934 -3.22228 galactic Per Second-epoch detections are separated by 2.3" and 8.1 pix
The object was found in VSX 1" V0661 Per
Type: SR:
# Max. Min./Amp. JD0 Period
13.500 V 14.200 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:05:05.77 +58:16:23.4: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:05:05.77 +58:16:23.4: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 05 05.77 +58 16 23.4 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0661 Per,2461199.8322,9.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0661 Per 20260608.3322 9.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.18 02:32:25.11 +58:26:07.8
135.83904 -1.88279 galactic Per Second-epoch detections are separated by 3.4" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:32:25.11 +58:26:07.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:25.11 +58:26:07.8: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:25.11 +58:26:07.8: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 25.11 +58 26 07.8 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.57 02:33:34.78 +57:08:52.6
136.47443 -3.01362 galactic Per Second-epoch detections are separated by 2.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.3948+57.1482 | 02:33:34.77 +57:08:53.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.942+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:34.78 +57:08:52.6: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:34.78 +57:08:52.6: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 34.78 +57 08 52.6 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.3948+57.1482,2461199.8322,9.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.3948+57.1482 20260608.3322 9.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.33 01:27:44.41 +62:06:39.4
127.16336 -0.46218 galactic Cas Second-epoch detections are separated by 1.5" and 7.3 pix
The object was found in VSX 2" NSVS 1696374
Type: SR
# Max. Min./Amp. JD0 Period
11.950 R1 12.250 R1 2451454.00000 193.000000000000 : C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:44.41 +62:06:39.4: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:44.41 +62:06:39.4: 13.96 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 27 44.41 +62 06 39.4 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1696374,2461199.8322,10.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1696374 20260608.3322 10.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.91 01:41:47.10 +59:03:46.9
129.37424 -3.17752 galactic Cas Second-epoch detections are separated by 1.7" and 7.4 pix
The object was found in VSX 1" ASASSN-V J014146.93+590346.7
Type: SR
# Max. Min./Amp. JD0 Period
13.670 V 14.220 V 2457304.00000 93.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:47.10 +59:03:46.9: 11.57 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:47.10 +59:03:46.9: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 41 47.10 +59 03 46.9 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J014146.93+590346.7,2461199.8322,9.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J014146.93+590346.7 20260608.3322 9.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.76 02:19:16.67 +59:42:21.1
133.80814 -1.29809 galactic Cas Second-epoch detections are separated by 0.8" and 8.2 pix
The object was found in VSX 1" ZTF J021916.76+594221.6
Type: SR
# Max. Min./Amp. JD0 Period
14.063 g Y 0.424 g 2458349.86040 72.477681200000 MS
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:16.67 +59:42:21.1: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:16.67 +59:42:21.1: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 19 16.67 +59 42 21.1 8.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J021916.76+594221.6,2461199.8322,8.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J021916.76+594221.6 20260608.3322 8.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.04 01:39:32.69 +64:53:03.9
128.01064 2.48810 galactic Cas Second-epoch detections are separated by 3.3" and 8.2 pix
The object was found in VSX 2" ASASSN-V J013932.54+645302.3
Type: YSO
# Max. Min./Amp. JD0 Period
12.800 g 16.100 g
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:32.69 +64:53:03.9: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:32.69 +64:53:03.9: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 39 32.69 +64 53 03.9 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J013932.54+645302.3,2461199.8322,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J013932.54+645302.3 20260608.3322 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.97 02:14:25.04 +56:42:47.8
134.17414 -4.33633 galactic Per Second-epoch detections are separated by 1.5" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457025172169888384 | 02:14:25.03 +56:42:50.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.091+/-0.037 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:14:25.04 +56:42:47.8: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:14:25.04 +56:42:47.8: 11.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 14 25.04 +56 42 47.8 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457025172169888384,2461199.8322,8.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457025172169888384 20260608.3322 8.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.02 02:20:07.53 +56:21:00.9
135.03903 -4.42247 galactic Per Second-epoch detections are separated by 3.8" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.0163+56.3482 | 02:20:07.53 +56:21:00.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:07.53 +56:21:00.9: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:07.53 +56:21:00.9: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 20 07.53 +56 21 00.9 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.0163+56.3482,2461199.8322,10.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.0163+56.3482 20260608.3322 10.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.44 02:19:48.00 +56:25:10.7
134.97307 -4.37227 galactic Per Second-epoch detections are separated by 3.4" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458272499382317568 | 02:19:48.03 +56:25:07.5 (Gaia DR3) | S (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:48.00 +56:25:10.7: 12.20 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:48.00 +56:25:10.7: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 19 48.00 +56 25 10.7 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458272499382317568,2461199.8322,9.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458272499382317568 20260608.3322 9.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.32 02:34:13.06 +56:03:48.9
136.97437 -3.98033 galactic Per Second-epoch detections are separated by 8.0" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.5561+56.0631 | 02:34:13.47 +56:03:47.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:13.06 +56:03:48.9: 13.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:13.06 +56:03:48.9: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 13.06 +56 03 48.9 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.5561+56.0631,2461199.8322,9.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.5561+56.0631 20260608.3322 9.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.12 02:22:56.71 +57:11:44.4
135.11329 -3.49596 galactic Per Second-epoch detections are separated by 0.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.7523+57.1948 | 02:22:56.77 +57:11:44.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.065+/-0.038 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:56.71 +57:11:44.4: 9.80 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:56.71 +57:11:44.4: 10.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 22 56.71 +57 11 44.4 8.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.7523+57.1948,2461199.8322,8.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.7523+57.1948 20260608.3322 8.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.13 02:25:27.49 +56:21:40.8
135.73000 -4.15622 galactic Per Second-epoch detections are separated by 2.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457518642429176576 | 02:25:27.34 +56:21:38.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:27.49 +56:21:40.8: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:27.49 +56:21:40.8: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 25 27.49 +56 21 40.8 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457518642429176576,2461199.8322,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457518642429176576 20260608.3322 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.75 02:18:24.84 +58:37:26.7
134.06238 -2.35541 galactic Per Second-epoch detections are separated by 0.7" and 8.1 pix
The object was found in VSX 1" TSVSC1 TN-N311132011-556-86-2
Type: SR
# Max. Min./Amp. JD0 Period
13.035 r Y 0.802 r 2458469.04980 210.487596000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:24.84 +58:37:26.7: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:24.84 +58:37:26.7: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 18 24.84 +58 37 26.7 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TSVSC1 TN-N311132011-556-86-2,2461199.8322,9.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TSVSC1 TN-N311132011-556-86-2 20260608.3322 9.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.73 02:23:49.27 +56:41:24.8
135.40191 -3.92815 galactic Per Second-epoch detections are separated by 4.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458382381836763136 | 02:23:49.38 +56:41:25.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.324+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:49.27 +56:41:24.8: 11.19 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:49.27 +56:41:24.8: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 23 49.27 +56 41 24.8 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458382381836763136,2461199.8322,9.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458382381836763136 20260608.3322 9.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.06 02:34:03.25 +56:00:34.3
136.97420 -4.03901 galactic Per Second-epoch detections are separated by 6.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457322280826978560 | 02:34:03.58 +56:00:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:03.25 +56:00:34.3: 13.03 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:03.25 +56:00:34.3: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 34 03.25 +56 00 34.3 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457322280826978560,2461199.8322,9.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457322280826978560 20260608.3322 9.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.88 01:49:47.70 +65:03:21.5
129.03766 2.87831 galactic Cas Second-epoch detections are separated by 2.0" and 7.9 pix
The object was found in VSX 0" ASASSN-V J014947.64+650321.4
Type: SR
# Max. Min./Amp. JD0 Period
14.000 V 15.100 V 2458390.66790 121.379022800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:47.70 +65:03:21.5: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:47.70 +65:03:21.5: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 49 47.70 +65 03 21.5 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J014947.64+650321.4,2461199.8322,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J014947.64+650321.4 20260608.3322 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 6.74 01:43:36.46 +58:48:08.2
129.65676 -3.38663 galactic Cas Second-epoch detections are separated by 0.8" and 7.4 pix
The object was found in VSX 1" V0917 Cas
Type: SR:
# Max. Min./Amp. JD0 Period
10.500 V 11.200 V M7
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:36.46 +58:48:08.2: 12.52 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:36.46 +58:48:08.2: 10.36 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.36 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 43 36.46 +58 48 08.2 6.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0917 Cas,2461199.8322,6.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0917 Cas 20260608.3322 6.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.21 02:38:48.34 +57:57:34.8
136.80011 -1.99173 galactic Cas Second-epoch detections are separated by 1.7" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.7144+57.9584 | 02:38:48.32 +57:57:33.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.120+/-0.028 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:48.34 +57:57:34.8: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:48.34 +57:57:34.8: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 38 48.34 +57 57 34.8 9.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.7144+57.9584,2461199.8322,9.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.7144+57.9584 20260608.3322 9.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.43 01:24:30.70 +59:38:48.0
127.10497 -2.95684 galactic Cas Second-epoch detections are separated by 2.0" and 7.2 pix
The object was found in VSX 1" ASASSN-V J012430.51+593847.9
Type: SR
# Max. Min./Amp. JD0 Period
13.360 V 13.950 V 2458378.66340 139.847766200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:30.70 +59:38:48.0: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:30.70 +59:38:48.0: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 24 30.70 +59 38 48.0 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J012430.51+593847.9,2461199.8322,9.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J012430.51+593847.9 20260608.3322 9.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.91 02:27:22.11 +62:38:26.1
133.70318 1.79228 galactic Cas Second-epoch detections are separated by 0.5" and 8.4 pix
The object was found in VSX 0" V0937 Cas
Type: SR:
# Max. Min./Amp. JD0 Period
13.700 V 14.500 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:22.11 +62:38:26.1: 10.81 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:22.11 +62:38:26.1: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 22.11 +62 38 26.1 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0937 Cas,2461199.8322,9.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0937 Cas 20260608.3322 9.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.08 02:21:26.42 +57:16:57.3
134.89183 -3.48436 galactic Per Second-epoch detections are separated by 3.3" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.3797+57.2867 | 02:21:26.45 +57:16:55.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.400+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:26.42 +57:16:57.3: 11.52 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:26.42 +57:16:57.3: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 26.42 +57 16 57.3 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.3797+57.2867,2461199.8322,9.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.3797+57.2867 20260608.3322 9.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.46 02:27:55.31 +56:27:24.0
136.01425 -3.94453 galactic Per Second-epoch detections are separated by 0.6" and 8.2 pix
The object was found in VSX 2" ASASSN-V J022755.53+562722.6
Type: SRS
# Max. Min./Amp. JD0 Period
13.790 g Y 0.160 g 2458428.83700 25.028000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:55.31 +56:27:24.0: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:55.31 +56:27:24.0: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 27 55.31 +56 27 24.0 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J022755.53+562722.6,2461199.8322,9.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J022755.53+562722.6 20260608.3322 9.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.34 02:43:44.96 +60:25:27.3
136.36563 0.51537 galactic Cas Second-epoch detections are separated by 1.7" and 8.5 pix
The object was found in VSX 2" V0492 Cas
Type: LB:
# Max. Min./Amp. JD0 Period
14.400 R 15.600 R C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:43:44.96 +60:25:27.3: 12.15 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:43:44.96 +60:25:27.3: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 43 44.96 +60 25 27.3 9.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0492 Cas,2461199.8322,9.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0492 Cas 20260608.3322 9.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.27 02:33:40.23 +57:40:02.3
136.28593 -2.52943 galactic Per Second-epoch detections are separated by 1.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.4074+57.6734 | 02:33:40.23 +57:40:02.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.238+/-0.026 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:40.23 +57:40:02.3: 13.17 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:40.23 +57:40:02.3: 10.77 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.77 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 33 40.23 +57 40 02.3 8.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.4074+57.6734,2461199.8322,8.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.4074+57.6734 20260608.3322 8.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.52 02:17:25.67 +57:06:42.6
134.43572 -3.82684 galactic Per Second-epoch detections are separated by 2.2" and 8.3 pix
The object was found in VSX 1" Gaia DR3 458558819093050880
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.030 G 12.080 G 1.945390000000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:17:25.67 +57:06:42.6: 11.51 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:17:25.67 +57:06:42.6: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 17 25.67 +57 06 42.6 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458558819093050880,2461199.8322,9.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458558819093050880 20260608.3322 9.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 7.45 02:37:50.78 +57:54:15.9
136.70550 -2.09334 galactic Cas Second-epoch detections are separated by 0.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457950376842758784 | 02:37:50.90 +57:54:16.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB- 1959LS....C01....0H LS I +57 74 J-Ks=0.095+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:50.78 +57:54:15.9: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:50.78 +57:54:15.9: 9.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.96 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 37 50.78 +57 54 15.9 7.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457950376842758784,2461199.8322,7.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457950376842758784 20260608.3322 7.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.14 02:32:22.33 +58:28:54.9
135.81580 -1.84215 galactic Per Second-epoch detections are separated by 2.4" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.1041+58.4796 | 02:32:22.34 +58:28:55.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A3IV (LAMOST DR5) J-Ks=0.137+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:22.33 +58:28:54.9: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:22.33 +58:28:54.9: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 32 22.33 +58 28 54.9 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.1041+58.4796,2461199.8322,9.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.1041+58.4796 20260608.3322 9.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.39 02:21:36.06 +57:03:37.7
134.98834 -3.68568 galactic Per Second-epoch detections are separated by 1.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.3906+57.0654 | 02:21:36.07 +57:03:38.2 (Gaia DR3) | NSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.098+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:36.06 +57:03:37.7: 12.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:36.06 +57:03:37.7: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 21 36.06 +57 03 37.7 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.3906+57.0654,2461199.8322,9.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.3906+57.0654 20260608.3322 9.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.62 01:33:44.53 +60:46:20.5
128.07583 -1.67618 galactic Cas Second-epoch detections are separated by 3.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:33:44.53 +60:46:20.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:44.53 +60:46:20.5: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:44.53 +60:46:20.5: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 33 44.53 +60 46 20.5 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.02 00:53:38.56 +65:00:02.2
123.16501 2.12986 galactic Cas Second-epoch detections are separated by 1.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:53:38.56 +65:00:02.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:53:38.56 +65:00:02.2: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:53:38.56 +65:00:02.2: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 00 53 38.56 +65 00 02.2 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.8322,10.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.3322 10.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 10.45 02:02:57.28 +62:23:12.1
131.11342 0.65640 galactic Cas Second-epoch detections are separated by 2.2" and 8.2 pix
The object was found in VSX 5" ZTF J020256.84+622316.3
Type: RS
# Max. Min./Amp. JD0 Period
13.190 r Y 0.044 r 2458652.94840 1.972301600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:57.28 +62:23:12.1: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:57.28 +62:23:12.1: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 02 57.28 +62 23 12.1 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J020256.84+622316.3,2461199.8322,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J020256.84+622316.3 20260608.3322 10.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 8.30 02:31:45.85 +55:57:57.7
136.69420 -4.20163 galactic Per Second-epoch detections are separated by 6.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.9520+55.9630 | 02:31:46.12 +55:57:58.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.866+/-0.036 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:45.85 +55:57:57.7: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:45.85 +55:57:57.7: 10.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.96 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 45.85 +55 57 57.7 8.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.9520+55.9630,2461199.8322,8.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.9520+55.9630 20260608.3322 8.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.96 02:17:01.95 +56:44:19.3
134.50664 -4.19716 galactic Per Second-epoch detections are separated by 5.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J034.2591+56.7399 | 02:17:01.95 +56:44:19.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:17:01.95 +56:44:19.3: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:17:01.95 +56:44:19.3: 12.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 17 01.95 +56 44 19.3 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J034.2591+56.7399,2461199.8322,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J034.2591+56.7399 20260608.3322 9.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.37 01:52:19.58 +57:19:07.2
131.10877 -4.58325 galactic Per Second-epoch detections are separated by 1.7" and 7.6 pix
The object was found in VSX 1" BX Per
Type: LB
# Max. Min./Amp. JD0 Period
14.400 pg 15.000 pg M6
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:19.58 +57:19:07.2: 13.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:19.58 +57:19:07.2: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 52 19.58 +57 19 07.2 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BX Per,2461199.8322,9.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BX Per 20260608.3322 9.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.91 02:49:56.76 +63:51:39.5
135.54113 3.92926 galactic Cas Second-epoch detections are separated by 1.4" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 467697169465689088 | 02:49:53.99 +63:51:24.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.456+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:49:56.76 +63:51:39.5: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:49:56.76 +63:51:39.5: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 49 56.76 +63 51 39.5 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 467697169465689088,2461199.8322,9.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 467697169465689088 20260608.3322 9.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.32 02:29:48.78 +57:57:50.6
135.69769 -2.44859 galactic Per Second-epoch detections are separated by 2.4" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 458091698450291584 | 02:29:48.78 +57:57:49.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: A7V (LAMOST DR5) J-Ks=0.767+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:48.78 +57:57:50.6: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:48.78 +57:57:50.6: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 29 48.78 +57 57 50.6 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 458091698450291584,2461199.8322,9.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 458091698450291584 20260608.3322 9.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.99 02:31:31.28 +57:22:45.9
136.12854 -2.90546 galactic Per Second-epoch detections are separated by 3.9" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458018340407727104 | 02:31:29.87 +57:22:43.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M3.5 1985ApJS...59..197B LTT 10837
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:31.28 +57:22:45.9: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:31.28 +57:22:45.9: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 02 31 31.28 +57 22 45.9 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458018340407727104,2461199.8322,9.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458018340407727104 20260608.3322 9.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.3322 2461199.8322 9.75 01:43:45.33 +58:23:44.8
129.75774 -3.78091 galactic Cas Second-epoch detections are separated by 2.9" and 7.6 pix
The object was found in VSX 1" ASASSN-V J014345.26+582344.7
Type: SR
# Max. Min./Amp. JD0 Period
13.860 V 14.440 V 2458355.00070 93.081983100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:45.33 +58:23:44.8: 13.33 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:45.33 +58:23:44.8: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.3323* 01 43 45.33 +58 23 44.8 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J014345.26+582344.7,2461199.8322,9.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J014345.26+582344.7 20260608.3322 9.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461199.83332972 08.06.2026 07:59:49.688 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 165
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 17 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 29745
Objects passed selection criteria: 29639
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 22811
Average stars matched: 22118 (96.962 %)
Memory usage VmPeak: 132908 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 03:10:27 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461199.83332972 08.06.2026 07:59:49.688 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 953
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 96 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 202460
Objects passed selection criteria: 201978
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 153208
Average stars matched: 147670 (96.3859 %)
Memory usage VmPeak: 1957320 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 03:18:39 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
SExtractor catalog cache: saved Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461199.83116492
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits'
wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits
Image size: 942.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:46.456 +61:56:25.93 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:46.456 +61:56:25.93
Angular distance between the image centers 0.0566 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
Image size: 942.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:49.368 +61:57:06.84 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:49.368 +61:57:06.84
Angular distance between the image centers 0.0524 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:42:46.456 +61:56:25.93
Second-epoch second image center 01:42:49.368 +61:57:06.84
Angular distance between the image centers 0.01272 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.wd9zXP2laB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.e0TkIQXedz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits &> /tmp/tmp.eWJLg6VLpc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits &> /tmp/tmp.Mtwcba8mfG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.937800
a=0.000000 b=1.000000 c=22.937800
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.30
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.30
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=5.9)
Read 31681 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.0659 to 45.7628 deg, Dec +55.3336 to +67.4023 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.0659 to 45.7628 deg, Dec 55.3336 to 67.4023 deg
Loaded 26179 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 14497 out of 16269 total matches.
Matched with Tycho-2 16269 out of 31681 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 111 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
4.3 pix fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits
2.6 pix fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
2.2 pix wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
15.3 mag. Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
15.3 mag. Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
13.8 mag. fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits
14.2 mag. fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.wd9zXP2laB (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3786, passed=31559
Got 31559 stars (including 27744 good ones) from the SExtractor catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 31559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 364 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 280 matched stars entering correct_measured_positions(), 228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 267 matched stars entering correct_measured_positions(), 10048 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 403 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 336 matched stars entering correct_measured_positions(), 10093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.39"
Accuracy estimation diagnostic: 331 matched stars entering correct_measured_positions(), 12854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.75"
Excluding outliers - 331 stars left (next iteration limit 293)
WCS_QUALITY_DIAG: file=Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=331 sigma_overall_arcsec=7.291 sigma_q1_arcsec=27.811 sigma_q2_arcsec=12.006 sigma_q3_arcsec=24.661 sigma_q4_arcsec=4.199 n_q1=15 n_q2=98 n_q3=37 n_q4=181 worst_quadrant_to_overall_ratio=3.814
The image catalog is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.e0TkIQXedz (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3692, passed=31681
Got 31681 stars (including 27947 good ones) from the SExtractor catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 31681 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits N_match=973 sigma_overall_arcsec=0.406 sigma_q1_arcsec=0.531 sigma_q2_arcsec=0.401 sigma_q3_arcsec=0.378 sigma_q4_arcsec=0.344 n_q1=119 n_q2=244 n_q3=303 n_q4=307 worst_quadrant_to_overall_ratio=1.308
The image catalog is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.eWJLg6VLpc (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits
Checking if the catalog wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits
WCS catalog name: wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits.cat
SExtractor catalog parsing summary: zero_flux=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=766, passed=13956
Got 13956 stars (including 13184 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits.cat
util/solve_plate_with_UCAC5 got 13956 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.5'
Seting catalog search parameters based on the expected field of view 942.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013090 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010472 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 13557 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 13557 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 13539 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 964 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits N_match=964 sigma_overall_arcsec=0.456 sigma_q1_arcsec=0.490 sigma_q2_arcsec=0.467 sigma_q3_arcsec=0.347 sigma_q4_arcsec=0.510 n_q1=279 n_q2=284 n_q3=241 n_q4=160 worst_quadrant_to_overall_ratio=1.118
The image catalog is written to wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits -region wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Mtwcba8mfG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
Checking if the catalog wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
WCS catalog name: wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=969, passed=14623
Got 14623 stars (including 13641 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits.cat
util/solve_plate_with_UCAC5 got 14623 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010473 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 14179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 14179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 14179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits N_match=967 sigma_overall_arcsec=0.381 sigma_q1_arcsec=0.394 sigma_q2_arcsec=0.405 sigma_q3_arcsec=0.320 sigma_q4_arcsec=0.321 n_q1=285 n_q2=321 n_q3=225 n_q4=136 worst_quadrant_to_overall_ratio=1.062
The image catalog is written to wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits -region wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits sigma_overall=7.291 worst_q_ratio=3.814
ref2=Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits sigma_overall=0.406 worst_q_ratio=1.308
new1=fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits sigma_overall=0.456 worst_q_ratio=1.118
new2=fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits sigma_overall=0.381 worst_q_ratio=1.062
reference average sigma_overall=3.8485 worst_q_ratio=2.561
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278_astrometric_residuals.png (see messages above)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-56-42_20.00sec_0.00C_LIGHTs_0277.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cas-03-Q1b1x1_030123_TTUQ1b1x1_4022728_3msOlQbH/wcs_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278.fits'
Preparing the HTML report for the field Cas-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:03.60 +56:50:28.7: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:03.60 +56:50:28.7: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 02:31:03.60 +56:50:28.7: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:45.30 +55:56:54.2: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:30.46 +56:11:02.0: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:27.60 +56:46:56.1: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:45.30 +55:56:54.2: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 02:30:45.30 +55:56:54.2: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:09.05 +56:37:12.1: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:27.60 +56:46:56.1: 9.64 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:37.81 +57:29:13.3: 15.75 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 9.64 +/- 0.00
Forced photometry filter REJECTED candidate at 02:25:27.60 +56:46:56.1: ref_mag=9.64 +/- 0.00 new_mean_mag=9.5055 delta=0.14 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:30.46 +56:11:02.0: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 02:21:30.46 +56:11:02.0: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:09.05 +56:37:12.1: 9.21 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:10.28 +56:27:12.5: 15.70 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 9.21 +/- 0.00
Forced photometry filter REJECTED candidate at 02:29:09.05 +56:37:12.1: ref_mag=9.21 +/- 0.00 new_mean_mag=9.3734 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:24.36 +56:23:03.7: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:37.81 +57:29:13.3: 9.60 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.60 +/- 0.00
Forced photometry filter REJECTED candidate at 02:35:37.81 +57:29:13.3: ref_mag=9.60 +/- 0.00 new_mean_mag=9.7371 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:11.88 +56:35:43.1: 10.93 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:10.28 +56:27:12.5: 9.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.54 +/- 0.00
Forced photometry filter REJECTED candidate at 02:29:10.28 +56:27:12.5: ref_mag=9.54 +/- 0.00 new_mean_mag=9.6614 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:24.36 +56:23:03.7: 9.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.59 +/- 0.00
Forced photometry filter REJECTED candidate at 02:27:24.36 +56:23:03.7: ref_mag=9.59 +/- 0.00 new_mean_mag=9.7969 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:44.17 +56:06:07.1: 13.99 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:26.40 +56:06:42.2: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:11.88 +56:35:43.1: 9.75 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:54.08 +56:16:37.2: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:55.20 +56:25:08.5: 15.80 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 9.85 +/- 0.00
Forced photometry filter REJECTED candidate at 02:24:11.88 +56:35:43.1: ref_mag=9.85 +/- 0.00 new_mean_mag=9.9084 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:44.17 +56:06:07.1: 9.66 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.66 +/- 0.00
Forced photometry filter REJECTED candidate at 02:34:44.17 +56:06:07.1: ref_mag=9.66 +/- 0.00 new_mean_mag=9.8783 delta=-0.22 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:44.94 +56:56:12.6: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:35.38 +56:18:13.8: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:13.55 +56:15:03.7: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:26.40 +56:06:42.2: 10.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.02 +/- 0.00
Forced photometry filter REJECTED candidate at 02:23:26.40 +56:06:42.2: ref_mag=10.02 +/- 0.00 new_mean_mag=10.0633 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:05.72 +57:22:03.5: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:54.08 +56:16:37.2: 10.58 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:55.20 +56:25:08.5: 9.98 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.58 +/- 0.00
Forced photometry reference-image weighted average: 9.98 +/- 0.00
Forced photometry filter REJECTED candidate at 02:21:55.20 +56:25:08.5: ref_mag=9.98 +/- 0.00 new_mean_mag=10.1583 delta=-0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:20:54.08 +56:16:37.2: ref_mag=10.58 +/- 0.00 new_mean_mag=10.3116 delta=0.27 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:44.94 +56:56:12.6: 10.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.11 +/- 0.00
Forced photometry filter REJECTED candidate at 02:30:44.94 +56:56:12.6: ref_mag=10.11 +/- 0.00 new_mean_mag=10.2487 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:35.38 +56:18:13.8: 10.30 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.30 +/- 0.00
Forced photometry filter REJECTED candidate at 02:22:35.38 +56:18:13.8: ref_mag=10.30 +/- 0.00 new_mean_mag=10.3075 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:13.55 +56:15:03.7: 9.91 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:35:13.55 +56:15:03.7: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:05.72 +57:22:03.5: 10.19 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.19 +/- 0.00
Forced photometry filter REJECTED candidate at 02:32:05.72 +57:22:03.5: ref_mag=10.19 +/- 0.00 new_mean_mag=10.1496 delta=0.04 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:06.89 +56:07:52.9: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:10.19 +56:24:23.5: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:01.73 +57:02:07.9: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:06.89 +56:07:52.9: 10.47 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.47 +/- 0.00
Forced photometry filter REJECTED candidate at 02:22:06.89 +56:07:52.9: ref_mag=10.47 +/- 0.00 new_mean_mag=10.4253 delta=0.05 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:28.19 +56:11:20.3: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:20.39 +56:12:12.8: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:04.53 +57:10:37.9: 13.36 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:10.19 +56:24:23.5: 10.43 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.43 +/- 0.00
Forced photometry filter REJECTED candidate at 02:22:10.19 +56:24:23.5: ref_mag=10.43 +/- 0.00 new_mean_mag=10.5274 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:01.73 +57:02:07.9: 10.81 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.81 +/- 0.00
Forced photometry filter REJECTED candidate at 02:33:01.73 +57:02:07.9: ref_mag=10.81 +/- 0.00 new_mean_mag=10.5058 delta=0.30 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:45.24 +57:08:08.1: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:32.09 +56:10:00.5: 15.58 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:28.19 +56:11:20.3: 10.37 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.37 +/- 0.00
Forced photometry filter REJECTED candidate at 02:25:28.19 +56:11:20.3: ref_mag=10.37 +/- 0.00 new_mean_mag=10.5504 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:20.39 +56:12:12.8: 10.43 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.43 +/- 0.00
Forced photometry filter REJECTED candidate at 02:25:20.39 +56:12:12.8: ref_mag=10.43 +/- 0.00 new_mean_mag=10.5873 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:04.53 +57:10:37.9: 10.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.67 +/- 0.01
Forced photometry filter REJECTED candidate at 02:22:04.53 +57:10:37.9: ref_mag=10.67 +/- 0.01 new_mean_mag=10.6842 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:42.88 +56:07:10.9: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:45.24 +57:08:08.1: 10.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.52 +/- 0.00
Forced photometry filter REJECTED candidate at 02:32:45.24 +57:08:08.1: ref_mag=10.52 +/- 0.00 new_mean_mag=10.5759 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:32.09 +56:10:00.5: 10.60 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.60 +/- 0.00
Forced photometry filter REJECTED candidate at 02:20:32.09 +56:10:00.5: ref_mag=10.60 +/- 0.00 new_mean_mag=10.6817 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:07.71 +56:33:53.1: 15.18 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:42.88 +56:07:10.9: 10.59 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:25.85 +56:07:05.4: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:12.04 +57:09:47.8: 15.81 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 10.59 +/- 0.00
Forced photometry filter REJECTED candidate at 02:23:42.88 +56:07:10.9: ref_mag=10.59 +/- 0.00 new_mean_mag=10.6813 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:07.71 +56:33:53.1: 10.68 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.68 +/- 0.00
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:04.82 +56:49:24.8: 15.73 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 02:27:07.71 +56:33:53.1: ref_mag=10.68 +/- 0.00 new_mean_mag=10.6720 delta=0.01 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:33.89 +56:34:21.8: 13.98 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:25.85 +56:07:05.4: 10.36 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.36 +/- 0.00
Forced photometry filter REJECTED candidate at 02:31:25.85 +56:07:05.4: ref_mag=10.36 +/- 0.00 new_mean_mag=10.3677 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:51.90 +57:04:09.8: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:12.04 +57:09:47.8: 10.76 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.76 +/- 0.00
Forced photometry filter REJECTED candidate at 02:31:12.04 +57:09:47.8: ref_mag=10.76 +/- 0.00 new_mean_mag=10.6884 delta=0.07 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:06.49 +56:29:59.8: 15.38 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:50.68 +56:20:49.5: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:35.03 +57:36:36.5: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:04.82 +56:49:24.8: 10.34 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:33.89 +56:34:21.8: 10.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.34 +/- 0.00
Forced photometry reference-image weighted average: 10.60 +/- 0.00
Forced photometry filter REJECTED candidate at 02:25:33.89 +56:34:21.8: ref_mag=10.60 +/- 0.00 new_mean_mag=10.6954 delta=-0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:32:04.82 +56:49:24.8: ref_mag=10.34 +/- 0.00 new_mean_mag=10.5419 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:51.90 +57:04:09.8: 10.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.54 +/- 0.00
Forced photometry filter REJECTED candidate at 02:30:51.90 +57:04:09.8: ref_mag=10.54 +/- 0.00 new_mean_mag=10.6852 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:48.60 +57:01:45.6: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:06.49 +56:29:59.8: 10.87 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:50.68 +56:20:49.5: 10.59 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:35.03 +57:36:36.5: 10.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.87 +/- 0.00
Forced photometry reference-image weighted average: 10.59 +/- 0.00
Forced photometry filter REJECTED candidate at 02:24:06.49 +56:29:59.8: ref_mag=10.87 +/- 0.00 new_mean_mag=10.8767 delta=-0.00 (need > 0.90)
Forced photometry reference-image weighted average: 10.71 +/- 0.00
Forced photometry filter REJECTED candidate at 02:28:50.68 +56:20:49.5: ref_mag=10.59 +/- 0.00 new_mean_mag=10.5850 delta=0.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:36:35.03 +57:36:36.5: ref_mag=10.71 +/- 0.00 new_mean_mag=10.7937 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:04.74 +56:15:32.3: 15.13 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:48.60 +57:01:45.6: 10.42 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.42 +/- 0.00
Forced photometry filter REJECTED candidate at 02:33:48.60 +57:01:45.6: ref_mag=10.42 +/- 0.00 new_mean_mag=10.6406 delta=-0.22 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:07.35 +56:25:11.9: 13.76 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:20.23 +57:29:30.1: 14.98 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:33.03 +56:53:09.2: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:04.74 +56:15:32.3: 11.01 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:31.55 +56:14:10.8: 15.78 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.02 +/- 0.01
Forced photometry filter REJECTED candidate at 02:21:04.74 +56:15:32.3: ref_mag=11.02 +/- 0.01 new_mean_mag=10.9714 delta=0.04 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:13.46 +56:36:46.9: 15.27 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:20.23 +57:29:30.1: 10.86 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.87 +/- 0.00
Forced photometry filter REJECTED candidate at 02:35:20.23 +57:29:30.1: ref_mag=10.87 +/- 0.00 new_mean_mag=10.9038 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:59.08 +56:30:01.5: 13.66 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:07.35 +56:25:11.9: 10.82 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:56.52 +56:13:25.8: 15.66 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Forced photometry filter REJECTED candidate at 02:26:07.35 +56:25:11.9: ref_mag=10.83 +/- 0.00 new_mean_mag=10.9544 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:33.03 +56:53:09.2: 10.78 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.78 +/- 0.00
Forced photometry filter REJECTED candidate at 02:30:33.03 +56:53:09.2: ref_mag=10.78 +/- 0.00 new_mean_mag=10.9158 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:31.55 +56:14:10.8: 10.86 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.86 +/- 0.00
Forced photometry filter REJECTED candidate at 02:22:31.55 +56:14:10.8: ref_mag=10.86 +/- 0.00 new_mean_mag=10.9980 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:13.46 +56:36:46.9: 10.79 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.79 +/- 0.00
Forced photometry filter REJECTED candidate at 02:26:13.46 +56:36:46.9: ref_mag=10.79 +/- 0.00 new_mean_mag=10.9390 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:18.60 +55:53:51.2: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:16.86 +55:42:14.2: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:59.08 +56:30:01.5: 11.39 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:56.52 +56:13:25.8: 10.95 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.01
Forced photometry reference-image weighted average: 10.95 +/- 0.00
Forced photometry filter REJECTED candidate at 02:19:56.52 +56:13:25.8: ref_mag=10.95 +/- 0.00 new_mean_mag=11.0480 delta=-0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:21:59.08 +56:30:01.5: ref_mag=11.42 +/- 0.01 new_mean_mag=11.1232 delta=0.30 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:13.31 +56:30:31.3: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:16.86 +55:42:14.2: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 02:35:16.86 +55:42:14.2: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:18.60 +55:53:51.2: 10.76 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.76 +/- 0.00
Forced photometry filter REJECTED candidate at 02:31:18.60 +55:53:51.2: ref_mag=10.76 +/- 0.00 new_mean_mag=10.8370 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:28.56 +56:33:05.9: 15.19 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:13.31 +56:30:31.3: 10.82 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:33.11 +56:13:10.0: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 10.82 +/- 0.00
Forced photometry filter REJECTED candidate at 02:25:13.31 +56:30:31.3: ref_mag=10.82 +/- 0.00 new_mean_mag=10.9710 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:45.74 +55:57:58.1: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:10.79 +56:48:28.8: 12.63 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:28.56 +56:33:05.9: 10.91 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.91 +/- 0.00
Forced photometry filter REJECTED candidate at 02:29:28.56 +56:33:05.9: ref_mag=10.91 +/- 0.00 new_mean_mag=11.0723 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:33.11 +56:13:10.0: 10.62 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.64 +/- 0.00
Forced photometry filter REJECTED candidate at 02:27:33.11 +56:13:10.0: ref_mag=10.64 +/- 0.00 new_mean_mag=10.8203 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:55.74 +56:30:20.3: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:09.10 +57:00:38.5: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:40.69 +57:26:09.8: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:45.74 +55:57:58.1: 10.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.96 +/- 0.00
Forced photometry filter REJECTED candidate at 02:31:45.74 +55:57:58.1: ref_mag=10.96 +/- 0.00 new_mean_mag=10.9320 delta=0.03 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:10.79 +56:48:28.8: 11.09 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.00
Forced photometry filter REJECTED candidate at 02:26:10.79 +56:48:28.8: ref_mag=11.17 +/- 0.00 new_mean_mag=11.1561 delta=0.01 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:55.74 +56:30:20.3: 11.04 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.04 +/- 0.00
Forced photometry filter REJECTED candidate at 02:26:55.74 +56:30:20.3: ref_mag=11.04 +/- 0.00 new_mean_mag=11.1254 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:52.90 +56:54:19.4: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:09.10 +57:00:38.5: 10.93 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.93 +/- 0.00
Forced photometry filter REJECTED candidate at 02:33:09.10 +57:00:38.5: ref_mag=10.93 +/- 0.00 new_mean_mag=11.0745 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:40.69 +57:26:09.8: 11.14 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.14 +/- 0.00
Forced photometry filter REJECTED candidate at 02:33:40.69 +57:26:09.8: ref_mag=11.14 +/- 0.00 new_mean_mag=11.2369 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:32.99 +55:57:16.2: 15.65 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:43.22 +56:24:12.6: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:59.51 +56:29:42.5: 15.65 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:52.90 +56:54:19.4: 11.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.07 +/- 0.01
Forced photometry filter REJECTED candidate at 02:30:52.90 +56:54:19.4: ref_mag=11.07 +/- 0.01 new_mean_mag=11.2021 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:08.67 +57:36:14.8: 15.72 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:32.99 +55:57:16.2: 10.84 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.84 +/- 0.00
Forced photometry filter REJECTED candidate at 02:29:32.99 +55:57:16.2: ref_mag=10.84 +/- 0.00 new_mean_mag=11.0003 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:43.22 +56:24:12.6: 11.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.01
Forced photometry filter REJECTED candidate at 02:26:43.22 +56:24:12.6: ref_mag=11.11 +/- 0.01 new_mean_mag=11.2136 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:59.51 +56:29:42.5: 11.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.13 +/- 0.01
Forced photometry filter REJECTED candidate at 02:27:59.51 +56:29:42.5: ref_mag=11.13 +/- 0.01 new_mean_mag=11.2841 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:04.63 +57:26:53.0: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:08.67 +57:36:14.8: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.41 +/- 0.01
Forced photometry filter REJECTED candidate at 02:35:08.67 +57:36:14.8: ref_mag=11.41 +/- 0.01 new_mean_mag=11.3161 delta=0.09 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:40.18 +57:40:02.6: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:04.63 +57:26:53.0: 11.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.39 +/- 0.01
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.09 +59:15:33.9: 15.94 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 02:35:04.63 +57:26:53.0: ref_mag=11.39 +/- 0.01 new_mean_mag=11.3638 delta=0.03 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:40.18 +57:40:02.6: 10.76 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.76 +/- 0.00
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.09 +59:15:33.9: 9.75 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:33:40.18 +57:40:02.6: ref_mag=10.76 +/- 0.00 new_mean_mag=10.9087 delta=-0.15 (need > 0.90)
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry filter KEPT candidate at 01:56:38.09 +59:15:33.9: ref_mag=9.75 +/- 0.00 new_mean_mag=8.6736 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:50.82 +57:54:15.7: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:28.97 +60:14:00.3: 14.73 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:29.85 +59:24:31.1: 15.67 +/- 0.31 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:50.82 +57:54:15.7: 9.93 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.93 +/- 0.00
Forced photometry filter REJECTED candidate at 02:37:50.82 +57:54:15.7: ref_mag=9.93 +/- 0.00 new_mean_mag=10.0052 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:56.65 +57:11:45.4: 11.41 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:28.97 +60:14:00.3: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter KEPT candidate at 01:16:28.97 +60:14:00.3: ref_mag=12.33 +/- 0.01 new_mean_mag=11.1341 delta=1.20 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:40.72 +60:54:41.9: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:29.85 +59:24:31.1: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry filter KEPT candidate at 02:24:29.85 +59:24:31.1: ref_mag=11.92 +/- 0.01 new_mean_mag=10.7948 delta=1.12 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:56.65 +57:11:45.4: 10.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.01 +/- 0.01
Forced photometry filter REJECTED candidate at 02:22:56.65 +57:11:45.4: ref_mag=11.01 +/- 0.01 new_mean_mag=10.6625 delta=0.35 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:40.72 +60:54:41.9: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Forced photometry filter KEPT candidate at 02:21:40.72 +60:54:41.9: ref_mag=11.02 +/- 0.00 new_mean_mag=9.4040 delta=1.61 (need > 0.90)
Adding exclusion_list_local.txt__out12304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20109.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 52188_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52188_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:25:58.11 +56:06:09.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52189_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52189_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52190_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52190_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:30:05.05 +56:40:24.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52194_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52194_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:22:56.84 +56:21:07.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52197_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52197_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:36:59.83 +63:08:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52199_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52199_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52200_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52200_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:55.55 +56:35:49.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52204_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52204_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:21:10.37 +56:09:52.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52207_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52207_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:24:41.62 +56:26:14.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52212_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52212_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:31:19.53 +56:53:52.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52218_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52218_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:33:16.43 +57:14:05.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52221_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52221_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 52222_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52222_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52226_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52226_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 52230_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52230_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52232_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52232_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:33:24.45 +56:01:05.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52233_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52233_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52239_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52239_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52246_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52246_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 52257_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52257_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:13.31 +56:42:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52260_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52260_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52262_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52262_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52265_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52265_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:56.90 +56:38:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52271_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52271_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 52274_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52274_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52278_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52278_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52282_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52282_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52286_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52286_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52296_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52296_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52299_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52299_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52318_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52318_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52324_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52324_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52327_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52327_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52328_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52328_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52330_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52330_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52339_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52339_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:29:45.54 +56:46:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52346_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52346_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52347_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52347_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:18:49.85 +57:07:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52354_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52354_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 52355_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52355_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:34:27.02 +64:32:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52358_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52358_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52359_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52359_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52362_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52362_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 52368_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52368_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:47.79 +56:36:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52372_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52372_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:23.97 +56:37:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52373_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52373_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:54.20 +56:38:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52375_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52375_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52379_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52379_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52380_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52380_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52384_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52384_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52385_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52385_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52386_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52386_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:23.06 +56:43:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52389_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52389_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52393_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52393_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52395_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52395_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52403_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52403_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52413_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52413_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:55.27 +56:49:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52416_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52416_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52418_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52418_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52426_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52426_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52440_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52440_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52441_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52441_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52442_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52442_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52451_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52451_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52453_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52453_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 52458_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52458_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52460_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52460_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:18.07 +56:48:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52466_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52466_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52469_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52469_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52475_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52475_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52482_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52482_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52486_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52486_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52488_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52488_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:49.04 +56:39:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52489_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52489_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52493_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52493_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52494_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52494_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52496_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52496_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52507_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52507_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:26:41.01 +60:46:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52513_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52513_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52521_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52521_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52531_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52531_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52532_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52532_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:29:19.74 +56:49:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52535_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52535_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:44.68 +56:50:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52538_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52538_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:58.04 +56:42:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52541_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52541_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52543_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52543_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52545_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52545_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52551_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52551_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52558_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52558_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52565_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52565_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:56.01 +56:44:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52568_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52568_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 52576_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52576_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52592_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52592_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52593_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52593_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52596_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52596_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52600_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52600_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 52603_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 52603_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 22224_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 22224_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 23009_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 23009_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:17:59.83 +57:53:59.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 02633_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 02633_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:15:23.79 +65:01:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20109_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 20109_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 27684_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 27684_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:06:39.56 +56:51:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26424_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 26424_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:51:53.10 +57:12:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23244_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 23244_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:01:28.14 +58:18:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20736_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 20736_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 18044_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 18044_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 17032_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 17032_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 23703_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 23703_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:54:54.02 +58:33:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50065_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 50065_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51449_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 51449_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:47:00.38 +65:27:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250674_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250674_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250678_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250678_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250681_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250681_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250686_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250686_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250691_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250691_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250692_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250692_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250698_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250698_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250700_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250700_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:43:10.64 +57:50:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250702_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250702_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250703_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250703_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250704_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250704_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250719_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250719_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250720_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250720_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250721_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250721_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250722_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250722_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250725_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250725_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:44:29.11 +57:52:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250727_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250727_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250729_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250729_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250737_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250737_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250739_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250739_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250740_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250740_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250743_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250743_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:53:55.11 +57:26:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250744_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250744_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250745_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250745_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250750_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250750_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250751_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250751_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250755_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250755_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250757_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250757_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250758_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250758_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250760_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250760_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250761_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250761_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250763_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250763_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250764_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250764_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250766_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250766_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250768_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250768_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250769_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250769_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250770_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250770_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250771_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250771_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250772_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250772_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:19:28.95 +57:13:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250773_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250773_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250775_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250775_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250776_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250776_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:55:14.63 +59:32:00.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250777_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250777_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250778_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250778_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:16:20.75 +62:42:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250779_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250779_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:42:46.24 +57:58:45.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250780_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250780_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250782_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250782_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250803_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250803_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:22:54.17 +56:37:24.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250804_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250804_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:33:32.80 +57:32:16.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250805_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250805_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:25:58.10 +56:06:09.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250806_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250806_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:30:04.96 +56:40:24.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250810_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250810_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:22:08.00 +57:06:49.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250811_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250811_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:22:56.82 +56:21:07.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250815_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250815_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:20:34.10 +56:19:49.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250816_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250816_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:32:24.81 +57:25:44.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250818_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250818_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:36:35.65 +57:43:13.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250819_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250819_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250821_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250821_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:55.54 +56:35:49.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250822_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250822_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250827_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250827_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:30:02.52 +57:14:56.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250828_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250828_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:32:52.80 +57:31:35.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250833_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250833_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:29:21.65 +57:05:22.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250834_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250834_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:21:10.38 +56:09:52.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250836_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250836_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:24:41.61 +56:26:14.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250838_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250838_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:31:19.53 +56:53:52.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250842_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250842_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:33:16.42 +57:14:04.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250843_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250843_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:48:46.89 +56:41:43.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250845_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250845_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:25:59.06 +56:39:27.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250846_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250846_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:34:58.69 +55:58:56.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250849_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250849_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:36:13.63 +57:43:40.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250850_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250850_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250853_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250853_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:22.01 +56:57:05.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250855_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250855_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:41.06 +57:11:21.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250860_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250860_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:33:24.47 +56:01:05.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250861_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250861_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250864_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250864_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250871_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250871_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250876_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250876_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250879_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250879_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250882_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250882_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250883_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250883_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250886_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250886_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250890_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250890_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250895_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250895_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:13.32 +56:42:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250896_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250896_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250897_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250897_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250899_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250899_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:56.91 +56:38:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250901_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250901_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 250909_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250909_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250911_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250911_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250914_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250914_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250918_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250918_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250919_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250919_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:40.63 +57:05:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250921_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250921_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250922_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250922_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:33.93 +56:48:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250928_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250928_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250930_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250930_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250933_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250933_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250934_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250934_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250937_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250937_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250939_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250939_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250943_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250943_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250946_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250946_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250955_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250955_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250959_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250959_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250961_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250961_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250964_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250964_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 250970_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250970_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250971_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250971_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250975_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250975_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:03.06 +56:50:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250976_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250976_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250982_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250982_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:29.16 +56:54:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250985_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250985_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 250987_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 250987_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:29:45.53 +56:46:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250996_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 250996_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251001_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251001_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 251002_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251002_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251003_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251003_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251004_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251004_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251007_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251007_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251009_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251009_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251010_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251010_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 251011_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251011_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251012_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251012_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251015_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251015_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251019_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251019_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251020_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251020_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:23.96 +56:37:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251022_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251022_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:54.21 +56:38:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251028_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251028_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:47.80 +56:36:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251029_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251029_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251033_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251033_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251034_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251034_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251035_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251035_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251039_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251039_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251042_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251042_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251044_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251044_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:23.08 +56:43:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251046_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251046_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251048_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251048_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251052_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251052_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251054_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251054_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251057_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251057_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251062_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251062_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251063_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251063_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251070_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251070_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251071_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251071_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251075_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251075_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251079_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251079_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:55.28 +56:49:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251080_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251080_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251082_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251082_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251083_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251083_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251085_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251085_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251087_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251087_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251093_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251093_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251104_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251104_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251107_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251107_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251109_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251109_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251111_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251111_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251114_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251114_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251115_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251115_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 251116_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251116_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251118_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251118_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251119_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251119_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251122_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251122_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251126_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251126_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251128_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251128_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251130_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251130_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:18.05 +56:48:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251131_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251131_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251136_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251136_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251138_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251138_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251143_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251143_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:46.33 +56:57:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251144_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251144_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251147_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251147_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251150_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251150_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:49.05 +56:39:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251154_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251154_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251156_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251156_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251157_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251157_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251158_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251158_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251160_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251160_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251162_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251162_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251169_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251169_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:26:41.05 +60:46:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251173_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251173_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251174_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251174_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251181_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251181_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251184_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251184_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251191_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251191_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251199_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251199_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:45.96 +57:08:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251200_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251200_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:29:19.73 +56:49:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251202_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251202_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251205_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251205_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251208_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251208_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251209_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251209_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251215_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251215_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251217_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251217_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251218_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251218_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:58.04 +56:42:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251219_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251219_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251221_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251221_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251225_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251225_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251226_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251226_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 251232_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251232_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251233_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251233_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:44.68 +56:50:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251237_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251237_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251248_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251248_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251251_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251251_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251253_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251253_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:57.37 +57:06:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251256_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251256_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:56.01 +56:44:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251260_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251260_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251261_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251261_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251269_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251269_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251273_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251273_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251278_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251278_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251281_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251281_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:38.43 +57:12:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251282_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251282_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251284_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251284_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251286_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251286_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251288_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251288_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251293_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251293_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251294_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251294_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251296_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251296_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251298_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251298_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251301_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251301_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251307_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251307_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:36.05 +56:56:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251310_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251310_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251313_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251313_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251319_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251319_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251320_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251320_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251324_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251324_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251327_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251327_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251328_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251328_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251332_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251332_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251338_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251338_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251344_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251344_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:01.24 +56:41:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251345_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251345_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251347_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251347_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251350_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251350_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:58.93 +56:39:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251351_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251351_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251355_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251355_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:56:38.50 +59:13:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251356_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251356_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:29:00.28 +56:46:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251360_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251360_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:27.53 +56:51:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251362_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251362_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251365_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251365_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:59.51 +56:50:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251368_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251368_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251370_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251370_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251372_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251372_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251375_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251375_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251377_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251377_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251378_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251378_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:43.60 +56:44:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251384_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251384_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251387_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251387_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251392_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251392_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251393_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251393_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251394_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251394_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251409_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251409_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:04.36 +57:06:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251410_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251410_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251415_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251415_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:49:48.24 +65:05:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251424_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251424_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251426_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251426_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251431_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251431_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251432_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251432_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251445_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251445_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 251446_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251446_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251453_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251453_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251455_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251455_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 251460_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251460_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251464_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251464_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251468_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251468_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 251469_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251469_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251470_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251470_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251471_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251471_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251472_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251472_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251473_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251473_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:00.75 +57:00:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251476_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251476_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251477_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251477_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:29:29.39 +56:57:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251479_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251479_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 251481_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251481_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:49.80 +56:52:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251488_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251488_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251490_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251490_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:53:16.27 +61:08:52.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251497_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251497_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:22:06.22 +56:34:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251498_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251498_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251499_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251499_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251502_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251502_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251506_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251506_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251512_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251512_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251521_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251521_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251523_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251523_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251526_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251526_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251527_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251527_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251533_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251533_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251535_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251535_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251536_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251536_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251537_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251537_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251538_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251538_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251540_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251540_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251541_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251541_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251543_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251543_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251544_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251544_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:03:46.98 +61:03:18.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251545_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251545_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251549_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251549_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:04.49 +56:59:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251553_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251553_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251559_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251559_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:50.19 +56:58:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251562_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251562_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251563_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251563_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:30.39 +57:10:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251565_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251565_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251568_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251568_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 251569_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251569_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251575_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251575_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:29:36.41 +56:40:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251581_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251581_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251589_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251589_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251592_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251592_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:45.28 +56:52:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251593_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251593_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251594_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251594_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251600_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251600_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:51:37.50 +62:56:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251603_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251603_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:38:00.53 +57:56:45.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251604_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251604_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251606_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251606_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251608_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251608_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251612_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251612_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251620_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251620_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251623_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251623_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251629_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251629_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251630_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251630_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251631_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251631_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251635_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251635_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251636_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251636_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:29:33.53 +56:51:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251637_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251637_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251638_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251638_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251641_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251641_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:29.98 +56:55:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251648_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251648_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251651_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251651_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251652_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251652_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251654_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251654_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251656_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251656_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251658_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251658_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:17:59.52 +57:47:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251661_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251661_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:32:19.45 +56:13:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251664_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251664_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:22.64 +56:52:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251672_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251672_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 251674_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251674_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:19:12.24 +65:36:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251676_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251676_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:48.68 +56:43:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251684_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251684_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251685_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251685_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251688_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251688_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251689_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251689_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251696_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251696_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251701_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251701_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 251711_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251711_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 251718_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251718_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251720_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251720_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251725_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251725_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:54.12 +56:50:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251727_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251727_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 251734_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251734_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:56.65 +56:52:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251735_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251735_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 251736_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251736_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251737_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251737_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251738_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251738_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:43.03 +56:57:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251739_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251739_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251741_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251741_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 251743_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251743_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251744_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251744_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:06.19 +57:03:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251748_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251748_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251751_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251751_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251760_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251760_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251761_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251761_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 251762_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251762_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251763_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251763_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251767_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251767_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251768_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251768_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 251771_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251771_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251772_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251772_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251780_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251780_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251783_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251783_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251791_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251791_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 251798_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251798_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251802_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251802_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251803_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251803_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251807_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251807_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251810_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251810_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251814_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251814_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251815_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251815_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:25:08.26 +56:38:29.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251819_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251819_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251820_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251820_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251823_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251823_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251830_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251830_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:24:00.24 +57:13:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251833_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251833_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251834_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251834_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251838_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251838_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:56:23.19 +59:10:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251839_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251839_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251840_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251840_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 251841_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251841_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:04:32.50 +57:59:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251848_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251848_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251855_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251855_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:31:15.70 +58:01:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251861_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251861_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251862_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251862_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251866_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251866_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251868_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251868_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251870_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251870_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251872_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251872_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251876_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251876_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251880_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251880_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:35:15.03 +63:00:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251881_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251881_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251885_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251885_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251891_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251891_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:14.80 +56:44:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251897_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251897_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251898_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251898_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:57.21 +57:03:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251900_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251900_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251904_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251904_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251910_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251910_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251912_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251912_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:26.74 +57:00:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251913_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251913_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251915_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251915_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 251918_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251918_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251919_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251919_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:36.85 +56:54:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251921_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251921_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 251923_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251923_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:37:21.90 +64:05:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251925_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251925_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251926_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251926_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251928_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251928_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:20.52 +56:44:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251930_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251930_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 251931_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251931_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251935_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251935_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251936_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251936_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:01.62 +57:00:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251939_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251939_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251940_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251940_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251947_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251947_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251950_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251950_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 251951_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251951_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251952_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251952_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:56:28.47 +60:47:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251955_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251955_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251957_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251957_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251959_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251959_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:05:03.76 +64:21:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251960_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251960_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251963_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251963_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 251968_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251968_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:05.01 +56:40:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251970_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251970_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:50:48.26 +64:16:20.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251971_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251971_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:12.73 +56:48:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251974_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251974_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 251977_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251977_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251983_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251983_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251984_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251984_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 251987_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 251987_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251999_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 251999_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 252006_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252006_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252011_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252011_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 252013_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252013_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252014_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252014_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252016_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252016_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252021_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252021_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252022_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252022_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252026_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252026_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252030_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252030_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252031_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252031_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252035_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252035_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252048_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252048_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252050_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252050_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252052_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252052_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252053_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252053_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252056_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252056_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252059_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252059_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:16:08.59 +58:49:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252065_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252065_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252070_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252070_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252074_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252074_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252077_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252077_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:40.86 +56:55:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252081_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252081_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 252082_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252082_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:21.14 +56:37:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252083_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252083_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252091_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252091_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252094_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252094_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252095_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252095_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252101_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252101_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252102_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252102_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:08:32.06 +63:35:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252105_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252105_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252107_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252107_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252110_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252110_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252111_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252111_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:14.99 +57:12:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252113_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252113_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252117_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252117_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252122_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252122_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252124_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252124_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252125_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252125_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252126_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252126_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252130_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252130_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 252134_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252134_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252140_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252140_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 252142_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252142_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252152_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252152_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 252153_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252153_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252155_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252155_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:56.19 +56:36:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252156_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252156_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:46.64 +57:11:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252165_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252165_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252166_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252166_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252171_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252171_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252173_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252173_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252174_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252174_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252182_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252182_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252188_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252188_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252189_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252189_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252190_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252190_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252196_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252196_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252199_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252199_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:51:03.01 +64:49:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252205_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252205_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252206_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252206_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252211_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252211_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 252212_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252212_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252213_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252213_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252224_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252224_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252229_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252229_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:54:01.05 +63:31:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252237_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252237_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252238_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252238_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252239_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252239_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252247_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252247_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252249_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252249_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:36:28.70 +62:40:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252251_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252251_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252252_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252252_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252255_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252255_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 252261_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252261_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252262_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252262_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:48:23.93 +65:06:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252266_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252266_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252267_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252267_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252270_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252270_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:23:23.66 +63:36:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252273_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252273_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252277_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252277_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252280_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252280_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252286_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252286_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252287_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252287_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 252289_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252289_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252294_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252294_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:43:03.44 +58:08:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252295_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252295_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252296_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252296_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252299_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252299_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:30:40.32 +56:40:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252300_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252300_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252304_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252304_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 252305_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252305_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:43.89 +57:06:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252308_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252308_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252311_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252311_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252312_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252312_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252316_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252316_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 252318_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252318_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252323_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252323_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252326_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252326_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252329_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252329_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:07:40.78 +63:30:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252330_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252330_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252337_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252337_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252338_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252338_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 252343_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252343_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252344_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252344_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252349_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252349_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252357_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252357_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:44:17.68 +61:53:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252359_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252359_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252363_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252363_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252365_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252365_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252367_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252367_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252371_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252371_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252374_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252374_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:27:52.88 +62:46:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252378_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252378_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:35:21.80 +56:08:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252379_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252379_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252380_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252380_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252386_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252386_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 252396_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252396_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:06:45.50 +59:50:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252397_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252397_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252399_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252399_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252401_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252401_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252403_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252403_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252406_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252406_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252408_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252408_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:00:35.85 +60:25:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252411_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252411_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:16:04.90 +58:49:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252413_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252413_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:00:37.19 +58:30:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252414_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252414_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252416_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252416_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252419_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252419_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252420_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252420_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252429_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252429_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252440_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252440_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252441_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252441_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:06:23.60 +62:44:01.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252448_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252448_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:39:57.18 +60:52:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252449_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252449_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252453_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252453_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252455_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252455_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252459_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252459_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252465_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252465_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:11:43.77 +66:29:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252467_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252467_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252473_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252473_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252483_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252483_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252486_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252486_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:37:44.91 +64:45:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252488_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252488_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252489_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252489_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 252494_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252494_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:00:53.31 +63:25:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252496_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252496_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252497_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252497_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:15:34.53 +59:17:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252503_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252503_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252505_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252505_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252506_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252506_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 252509_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252509_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252511_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252511_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252513_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252513_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:09.86 +56:55:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252518_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252518_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252521_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252521_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:25:59.71 +57:26:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252527_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252527_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252528_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252528_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:17:01.08 +61:40:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252531_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252531_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252534_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252534_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252538_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252538_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252539_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252539_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252547_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252547_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:35:50.53 +61:27:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252548_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252548_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 252549_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252549_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252552_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252552_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 252555_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252555_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252564_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252564_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:42:33.22 +63:52:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252567_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252567_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 252570_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252570_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252573_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252573_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252574_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252574_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252575_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252575_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:03.08 +56:49:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252582_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252582_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:45:14.74 +64:24:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252593_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252593_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 252608_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252608_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252609_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252609_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252612_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252612_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252618_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252618_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252620_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252620_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252623_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252623_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252625_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252625_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252641_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252641_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:45:07.86 +56:50:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252643_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252643_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252644_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252644_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252647_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252647_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 252650_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252650_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 252656_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252656_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252676_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252676_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 252681_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252681_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252684_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252684_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252691_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252691_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252693_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252693_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:35.01 +56:59:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252694_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252694_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252697_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252697_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252702_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252702_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:16:12.74 +62:42:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252706_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252706_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252709_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252709_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252715_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252715_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252716_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252716_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252725_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252725_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:38:12.05 +61:01:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252731_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252731_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252739_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252739_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252741_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252741_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252744_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252744_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252745_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252745_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252746_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252746_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252748_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252748_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:50.10 +62:54:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252749_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252749_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:47:18.82 +63:38:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252759_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252759_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252769_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252769_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252787_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252787_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252789_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252789_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252793_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252793_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252804_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252804_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 252818_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252818_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:20:13.89 +65:31:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252828_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252828_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:41:41.33 +57:56:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252835_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 252835_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:23:07.60 +61:11:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252843_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 252843_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 179380_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 179380_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:27:37.09 +56:48:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235843_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 235843_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 162337_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 162337_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 128268_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 128268_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 215315_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 215315_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
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Considering the candidate 208550_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 208550_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 214209_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 214209_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 134816_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 134816_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:24:29.86 +59:24:31.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 70687_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 70687_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:37:09.78 +61:55:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21138_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 21138_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:15:23.78 +65:01:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211999_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 211999_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:51:53.08 +57:12:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134840_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 134840_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 214517_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 214517_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:06:39.55 +56:51:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62860_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 62860_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:11:58.88 +63:39:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67097_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 67097_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:36:59.83 +63:08:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219961_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 219961_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 198104_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 198104_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 149973_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 149973_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 192577_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 192577_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 96282_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 96282_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 165523_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 165523_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 130602_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 130602_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 129356_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 129356_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:38:55.40 +59:02:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 179696_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 179696_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:29:57.19 +56:45:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34158_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 34158_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 216016_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 216016_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 34359_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 34359_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:34:27.13 +64:32:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213196_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 213196_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213664_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 213664_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 218015_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 218015_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184393_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 184393_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216928_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 216928_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157256_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 157256_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234806_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 234806_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196494_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 196494_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:01:28.13 +58:18:14.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215688_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 215688_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184872_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 184872_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:26:33.10 +57:05:12.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28797_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 28797_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201907_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 201907_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
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Considering the candidate 155598_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 155598_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154238_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 154238_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62555_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 62555_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185268_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 185268_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 39378_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:47:55.79 +64:32:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220590_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 220590_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150407_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 150407_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96078_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 96078_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 233881_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 233881_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:43.86 +58:26:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233764_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 233764_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:29:12.59 +56:59:41.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167698_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 167698_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177658_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 177658_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157757_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 157757_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148907_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 148907_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181535_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 181535_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125111_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 125111_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30951_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 30951_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193638_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 193638_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:28:52.27 +57:22:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156692_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 156692_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:56:38.11 +59:15:33.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 82358_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 82358_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193780_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 193780_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 00:54:53.95 +58:33:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213271_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 213271_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219398_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 219398_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218524_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 218524_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21028_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 21028_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163824_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 163824_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195946_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 195946_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42016_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 42016_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191949_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
Preparing report for the candidate 191949_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172562_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 172562_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:22:06.66 +56:36:16.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 92255_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 92255_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 01:00:48.96 +62:16:08.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163793_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278
The candidate 163793_fd_Cas-03-Q1b1x1_2026-06-08_02-59-49_20.00sec_-0.00C_LIGHTs_0278 did not pass the final checks
**** FOUND 02:31:26.84 +58:01:29.1 in the exclusion list exclusion_list_tycho2.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 44s
make_report_in_HTML.sh TOTAL: 2843s
Prepared the HTML report for the field Cas-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
02:21:40.72 +60:54:41.9
02:24:29.85 +59:24:31.1
01:16:28.97 +60:14:00.3
01:56:38.09 +59:15:33.9
01:33:44.53 +60:46:20.5
02:38:06.09 +59:06:42.5
02:19:16.67 +59:42:21.1
02:38:02.06 +58:50:39.8
02:32:22.33 +58:28:54.9
02:32:25.11 +58:26:07.8
01:24:30.70 +59:38:48.0
02:38:48.34 +57:57:34.8
02:18:24.84 +58:37:26.7
02:37:50.78 +57:54:15.9
02:32:59.26 +57:53:54.0
02:29:48.78 +57:57:50.6
01:41:47.10 +59:03:46.9
02:33:40.23 +57:40:02.3
02:17:25.67 +57:06:42.6
02:21:36.06 +57:03:37.7
02:22:56.71 +57:11:44.4
02:21:26.42 +57:16:57.3
01:43:45.33 +58:23:44.8
02:33:34.78 +57:08:52.6
02:31:31.28 +57:22:45.9
02:05:05.77 +58:16:23.4
01:43:36.46 +58:48:08.2
02:15:35.85 +56:21:36.3
02:49:56.76 +63:51:39.5
02:20:07.53 +56:21:00.9
02:31:45.85 +55:57:57.7
02:19:48.00 +56:25:10.7
02:34:03.25 +56:00:34.3
02:14:25.04 +56:42:47.8
02:25:27.49 +56:21:40.8
02:34:13.06 +56:03:48.9
01:52:19.58 +57:19:07.2
02:17:01.95 +56:44:19.3
02:25:13.30 +56:30:31.2
02:27:55.31 +56:27:24.0
02:23:49.27 +56:41:24.8
02:32:01.89 +57:03:30.5
02:28:33.48 +62:03:22.8
02:52:02.80 +63:39:30.2
01:59:42.41 +63:32:29.7
02:14:53.05 +64:11:56.5
02:08:06.43 +63:06:02.0
01:13:39.59 +63:12:31.2
01:00:19.87 +57:17:48.3
00:46:00.34 +57:56:20.1
00:37:39.91 +62:15:59.9
01:02:20.28 +57:02:48.2
01:08:39.11 +60:32:48.4
01:19:04.47 +60:02:34.1
00:47:54.55 +59:03:26.0
01:42:54.46 +61:13:30.6
02:52:09.97 +62:49:57.4
02:27:39.78 +57:06:42.3
02:30:58.90 +62:01:46.4
01:17:48.39 +57:17:35.2
01:57:25.08 +60:33:52.9
02:28:28.47 +58:25:05.6
02:37:12.84 +63:10:37.8
00:55:16.01 +57:59:06.5
00:56:47.59 +60:38:47.2
02:01:32.89 +65:05:48.8
01:59:56.21 +56:37:09.2
01:08:29.49 +57:06:54.4
00:52:55.06 +58:28:52.6
02:17:47.56 +56:14:45.2
02:36:02.71 +59:00:55.3
02:25:54.13 +56:38:48.5
02:18:52.86 +63:06:09.6
00:30:29.66 +66:05:42.3
02:19:40.58 +56:48:52.6
01:25:15.63 +64:40:33.5
00:46:11.73 +59:43:33.6
02:19:45.01 +56:50:30.5
02:20:35.00 +57:06:52.7
02:00:17.31 +65:03:54.9
02:20:50.58 +57:20:41.9
01:43:21.66 +56:52:28.8
00:36:54.99 +62:40:45.5
02:19:45.19 +57:01:14.5
02:29:09.04 +56:37:12.3
02:25:27.60 +56:46:56.1
02:34:10.54 +55:50:00.3
02:23:38.00 +56:52:44.8
02:22:03.76 +56:31:27.4
02:32:34.58 +57:29:15.3
02:34:00.78 +57:49:58.1
02:25:20.48 +56:51:13.6
02:29:10.13 +56:27:12.4
02:35:37.82 +57:29:13.2
02:27:24.37 +56:23:03.5
02:23:35.48 +56:34:27.4
02:34:44.20 +56:06:07.0
02:24:11.88 +56:35:43.2
02:33:34.76 +55:54:25.0
02:31:26.00 +55:59:07.0
02:18:01.26 +56:15:41.5
02:36:36.22 +57:46:58.9
02:19:46.68 +56:22:26.5
02:35:52.03 +57:47:22.2
02:23:26.41 +56:06:42.3
02:36:33.27 +57:54:38.9
02:21:55.20 +56:25:08.5
02:21:50.33 +56:34:31.6
02:20:54.08 +56:16:37.4
02:22:35.38 +56:18:13.9
02:34:44.93 +57:54:58.3
02:30:44.95 +56:56:12.6
02:32:05.73 +57:22:03.4
02:21:20.53 +56:29:12.7
02:24:43.66 +56:59:33.7
02:22:06.90 +56:07:52.9
02:37:36.88 +57:51:16.7
02:33:01.74 +57:02:07.9
02:19:52.93 +56:15:40.7
02:22:10.20 +56:24:23.3
02:19:48.61 +56:23:45.9
02:19:36.43 +56:14:20.7
02:27:48.55 +57:05:55.3
02:24:42.01 +56:55:47.8
02:32:45.26 +57:08:08.0
02:25:28.19 +56:11:20.2
02:25:20.40 +56:12:12.7
02:18:48.49 +56:17:54.8
02:23:42.88 +56:07:10.8
02:21:54.94 +56:42:38.7
02:20:55.04 +56:23:19.2
02:20:32.11 +56:10:00.6
02:27:07.72 +56:33:53.0
02:23:57.26 +57:12:24.5
02:31:12.06 +57:09:47.8
02:24:09.74 +56:34:02.3
02:22:04.60 +57:10:38.0
02:31:25.89 +56:07:05.1
02:32:04.83 +56:49:24.9
02:22:53.49 +56:47:13.1
02:33:49.40 +57:35:12.5
02:35:18.48 +57:31:39.8
02:30:51.91 +57:04:09.8
02:38:46.76 +57:49:57.1
02:25:33.89 +56:34:21.9
02:30:00.34 +57:28:19.7
02:28:50.69 +56:20:49.6
02:31:38.55 +57:13:46.4
02:36:35.03 +57:36:36.2
02:24:06.49 +56:29:59.8
02:24:33.46 +56:57:18.3
02:19:39.63 +56:20:11.8
02:29:17.13 +57:14:30.0
02:26:07.35 +56:25:11.7
02:21:55.92 +56:44:53.0
02:35:20.24 +57:29:29.9
02:19:45.17 +56:31:44.3
02:21:04.75 +56:15:32.3
02:30:33.01 +56:53:09.2
02:33:48.55 +57:01:45.9
02:31:18.70 +55:53:50.8
02:36:08.52 +57:39:33.9
02:30:32.25 +57:11:26.3
02:21:59.09 +56:30:01.6
02:25:03.15 +56:56:58.8
02:22:31.56 +56:14:10.7
02:24:18.81 +56:54:02.0
02:25:00.78 +56:51:31.9
02:19:56.52 +56:13:26.0
02:26:13.46 +56:36:46.9
02:27:33.11 +56:13:09.8
02:29:26.34 +57:23:02.8
02:23:02.19 +56:30:28.6
02:31:20.24 +57:33:46.4
02:24:32.63 +57:00:44.1
02:29:28.55 +56:33:06.0
02:16:52.43 +56:18:43.8
02:18:24.03 +56:23:21.4
02:26:55.75 +56:30:20.2
02:30:30.83 +57:30:27.8
02:23:48.03 +56:47:01.5
02:26:10.79 +56:48:28.8
02:33:09.10 +57:00:38.5
02:33:40.71 +57:26:09.7
02:36:22.58 +57:40:05.6
02:25:48.44 +56:55:12.4
02:23:17.91 +56:42:23.9
02:20:18.71 +56:31:49.5
02:21:34.57 +56:26:43.9
02:19:36.20 +56:23:21.9
02:25:56.01 +56:58:59.2
02:35:08.67 +57:36:14.5
02:37:50.64 +57:45:49.7
02:26:43.23 +56:24:12.4
02:35:04.64 +57:26:52.9
02:24:34.14 +56:53:00.2
02:22:27.95 +56:41:51.9
02:26:11.70 +56:56:03.6
02:18:05.24 +56:15:07.5
02:34:48.66 +57:38:04.9
02:27:59.53 +56:29:42.2
02:29:33.00 +55:57:16.1
02:24:02.04 +56:49:22.3
02:23:55.73 +56:44:45.5
02:21:52.12 +56:41:17.7
02:32:17.85 +57:17:09.3
02:23:38.21 +56:39:53.8
02:31:29.32 +57:11:54.7
02:37:50.68 +57:57:56.9
02:21:30.49 +57:12:34.5
02:25:30.12 +56:16:52.8
02:31:09.75 +57:16:14.4
02:20:07.36 +56:27:52.1
02:33:34.12 +55:49:25.9
02:33:03.26 +57:03:29.0
02:33:10.59 +57:32:53.7
02:36:59.45 +57:56:29.8
02:32:14.18 +55:56:22.8
02:25:56.75 +56:07:50.5
02:25:04.29 +56:13:07.5
02:33:34.41 +56:11:48.0
02:34:24.39 +57:28:26.1
02:38:13.42 +57:50:16.2
02:28:48.05 +56:30:07.8
02:33:54.63 +57:40:55.2
02:25:42.31 +56:37:12.9
02:21:55.06 +56:20:50.1
02:24:25.89 +56:32:55.3
02:24:47.99 +56:36:57.6
02:24:32.13 +56:43:35.2
02:26:15.82 +56:04:34.0
02:25:45.49 +56:26:32.2
02:21:36.86 +56:40:52.1
02:30:39.48 +57:13:42.2
02:25:07.44 +56:14:04.5
02:26:00.84 +56:46:18.0
02:26:59.49 +57:14:44.2
02:31:10.54 +57:30:46.6
02:29:57.33 +56:36:50.4
02:31:12.57 +57:00:49.3
02:20:24.56 +56:41:43.6
02:23:44.10 +56:55:56.9
02:23:14.27 +56:52:06.4
02:26:08.97 +56:16:06.3
02:33:43.78 +57:36:02.2
02:37:02.20 +57:41:39.3
02:33:51.00 +55:59:56.1
02:30:11.98 +57:38:18.7
02:21:27.44 +56:16:28.6
01:40:01.08 +60:52:38.4
02:26:02.37 +56:20:59.5
02:24:23.74 +56:54:04.6
02:24:38.20 +56:49:55.7
02:27:52.28 +56:29:28.8
02:25:32.87 +56:32:57.7
02:22:11.95 +56:20:47.3
02:33:49.02 +55:57:06.8
02:31:19.72 +56:52:39.5
02:30:19.30 +55:54:55.0
02:31:00.30 +56:00:28.1
02:25:11.80 +56:17:22.8
02:24:18.84 +56:19:49.3
02:25:48.43 +56:32:35.4
02:32:04.94 +56:53:51.4
02:32:35.29 +57:32:20.9
02:30:45.41 +57:06:28.3
02:35:26.60 +57:46:11.7
02:23:07.47 +56:41:44.4
02:30:51.81 +57:15:44.6
02:23:08.48 +56:20:24.9
02:30:16.92 +56:38:09.4
02:24:52.38 +56:43:10.9
02:35:34.92 +57:32:59.3
02:28:32.01 +56:00:36.5
02:24:53.93 +56:08:45.2
02:27:34.40 +56:16:53.2
02:36:55.81 +57:38:49.8
02:34:12.97 +56:11:54.0
02:20:11.71 +56:22:22.8
02:29:55.64 +56:55:49.6
02:30:33.48 +56:57:02.6
02:31:03.43 +55:52:01.6
02:20:25.25 +56:52:28.8
02:23:11.37 +56:11:21.3
02:26:55.66 +56:28:24.5
02:22:16.04 +56:22:42.6
02:27:23.12 +56:19:27.5
02:33:27.67 +57:14:45.0
02:24:46.87 +56:38:55.3
02:29:39.11 +56:11:33.0
02:37:01.15 +57:51:23.0
02:32:23.31 +57:38:37.3
02:24:38.57 +56:20:45.4
02:30:35.00 +56:43:58.4
02:31:51.45 +56:45:51.1
02:32:55.48 +57:08:54.0
02:34:13.94 +56:18:42.0
02:29:11.28 +57:21:01.0
02:27:53.71 +57:06:30.9
02:32:01.27 +56:51:17.5
02:33:37.69 +57:40:25.1
00:43:47.78 +61:53:59.7
02:32:47.65 +57:14:17.2
02:22:21.43 +56:34:19.1
02:32:49.40 +57:34:21.9
02:20:54.28 +56:36:05.4
02:22:22.77 +56:40:00.7
02:27:27.07 +56:31:10.2
02:21:52.46 +56:32:45.3
02:24:12.53 +56:49:25.8
02:21:33.10 +56:13:41.1
02:25:40.03 +56:29:20.6
02:21:38.53 +56:26:50.2
02:26:14.40 +56:12:13.5
02:39:23.99 +58:09:11.5
02:36:41.37 +57:37:08.5
02:35:58.35 +57:49:15.3
02:39:21.42 +58:07:09.8
02:29:41.54 +56:37:30.7
00:58:55.93 +58:04:05.2
02:33:30.94 +57:29:02.8
02:22:47.76 +56:11:09.8
02:21:19.11 +56:38:13.4
02:17:41.08 +56:28:32.5
02:28:01.17 +56:23:28.1
02:21:16.36 +56:23:43.0
02:24:58.44 +56:50:40.4
02:25:52.54 +57:02:04.3
02:27:42.18 +56:12:19.8
02:23:54.58 +56:06:52.8
01:58:16.63 +59:38:57.1
02:31:45.84 +57:14:33.1
02:17:50.40 +56:22:37.9
02:21:13.54 +56:28:44.7
02:24:21.26 +56:52:14.7
02:24:38.41 +56:48:43.1
02:34:31.90 +57:40:30.4
02:26:01.02 +56:28:14.9
02:23:57.17 +56:11:53.7
01:29:32.95 +61:46:25.0
02:34:04.49 +57:32:44.3
02:36:12.26 +57:41:56.0
02:28:09.05 +56:38:21.2
01:18:14.29 +61:44:36.0
02:31:47.11 +55:52:28.5
02:27:22.05 +56:31:18.8
02:37:15.58 +57:48:19.2
02:21:39.29 +56:31:44.8
02:33:11.11 +57:33:48.8
02:23:43.00 +56:38:37.8
02:20:52.81 +56:09:33.8
02:34:19.87 +57:08:33.3
00:36:55.91 +62:32:56.0
02:30:17.43 +56:43:02.2
02:28:44.08 +57:00:25.5
02:31:18.74 +57:03:50.9
02:18:56.21 +56:18:32.0
02:29:08.36 +57:12:16.0
02:23:53.85 +56:39:14.7
02:30:51.42 +57:16:48.8
02:35:42.02 +57:31:40.9
02:31:56.68 +57:24:00.2
02:38:19.87 +58:03:56.7
02:25:52.96 +56:47:30.0
02:33:08.29 +57:28:10.5
02:34:46.52 +57:13:22.5
02:30:07.17 +56:30:20.8
02:29:48.78 +56:41:55.8
02:26:58.18 +56:22:12.1
02:33:44.27 +56:59:34.7
02:33:03.94 +57:33:09.8
02:23:07.87 +56:29:01.2
02:25:56.53 +56:32:31.9
02:35:58.93 +57:32:00.1
02:27:44.66 +56:19:43.0
02:25:56.42 +57:04:40.2
02:31:02.85 +57:42:08.9
02:29:25.87 +55:58:55.7
02:31:52.57 +56:53:49.0
02:39:52.21 +58:24:37.9
02:27:18.72 +56:15:53.5
02:36:25.89 +57:52:58.9
02:24:27.20 +56:50:28.9
02:34:31.90 +56:11:08.8
02:27:31.55 +56:30:00.3
02:25:53.52 +56:14:35.6
02:30:58.33 +57:16:17.2
02:22:27.17 +56:43:56.9
02:24:37.23 +56:45:53.9
02:29:46.73 +56:03:52.6
02:24:29.35 +56:34:20.6
02:31:18.77 +57:16:22.0
02:31:20.63 +56:50:06.3
02:31:33.36 +57:25:43.5
02:21:07.65 +56:13:22.2
02:30:09.68 +57:23:15.1
02:33:18.10 +57:31:36.8
02:36:07.79 +57:32:58.9
02:34:41.26 +56:11:01.6
02:26:20.11 +57:00:45.6
02:30:53.15 +56:59:21.2
02:34:42.72 +57:17:58.8
02:27:57.88 +56:22:23.8
02:33:08.50 +57:21:20.2
02:37:52.11 +57:47:13.1
02:25:45.87 +56:22:47.0
02:38:14.42 +57:58:50.6
02:33:33.71 +57:37:46.7
02:21:35.29 +56:14:56.5
02:30:03.83 +56:36:39.2
02:26:36.42 +56:34:16.7
02:32:24.99 +57:27:18.3
02:29:29.43 +57:10:39.0
02:27:40.70 +56:20:28.5
02:34:04.61 +57:19:27.3
02:26:10.21 +56:21:10.3
02:22:29.14 +56:32:00.5
02:34:35.60 +57:34:23.2
02:34:46.10 +57:12:52.3
02:34:38.93 +57:26:15.3
02:32:54.63 +57:10:57.1
02:22:37.79 +56:37:17.0
02:23:18.87 +57:06:02.1
02:24:23.45 +56:13:56.3
02:20:23.58 +56:22:39.7
02:26:45.86 +56:23:26.2
02:30:55.12 +57:08:07.5
02:32:06.03 +57:05:00.6
02:25:39.55 +56:48:00.4
02:22:51.67 +56:24:33.0
02:25:12.20 +56:44:30.7
02:25:05.47 +56:20:33.3
02:25:48.30 +56:35:16.7
02:25:01.82 +56:15:07.5
02:32:01.41 +55:53:20.2
02:35:41.37 +57:27:01.8
02:24:54.82 +56:45:04.1
02:23:46.82 +57:05:04.4
02:27:24.28 +56:17:59.4
02:23:29.57 +56:10:15.1
02:34:46.00 +58:00:26.7
02:32:58.19 +57:38:43.0
02:37:47.78 +57:52:43.0
02:24:54.07 +56:55:39.8
02:37:58.92 +58:07:38.9
02:27:22.03 +56:50:16.1
02:36:17.73 +57:48:52.1
02:25:54.98 +56:55:26.7
02:27:32.20 +57:08:35.3
02:20:13.03 +56:15:34.8
02:22:27.81 +56:33:28.7
02:27:58.93 +57:31:01.3
02:33:32.05 +57:51:40.8
02:34:38.40 +57:44:07.3
02:25:47.88 +56:43:23.2
02:30:08.47 +57:20:50.2
02:38:25.27 +58:17:31.8
02:38:01.91 +58:25:43.4
02:22:07.92 +56:28:58.2
02:34:18.98 +56:07:35.1
02:27:20.09 +56:49:46.3
02:28:36.20 +56:28:40.0
02:23:45.93 +56:58:54.6
02:28:30.00 +56:31:48.6
02:28:30.82 +57:06:37.8
02:25:01.45 +56:33:15.8
02:30:19.39 +57:30:27.0
02:33:38.71 +57:12:31.9
02:32:02.17 +57:26:35.5
02:33:09.48 +57:50:43.7
02:24:54.81 +56:34:32.0
02:24:12.77 +56:08:04.7
02:24:25.62 +56:20:53.3
02:31:40.18 +57:12:25.9
02:21:22.21 +56:42:51.2
02:32:03.60 +57:19:01.2
02:29:35.90 +56:47:29.8
00:45:31.36 +61:20:32.6
02:24:19.17 +56:16:19.6
02:21:10.37 +56:34:16.2
02:25:03.41 +56:05:16.2
02:31:07.14 +56:54:53.9
02:29:01.50 +57:51:35.8
02:35:08.92 +57:20:11.7
02:38:11.28 +57:54:13.4
02:28:13.34 +57:23:00.9
01:31:48.44 +64:21:56.3
01:19:41.78 +62:51:03.2
02:37:45.34 +58:30:48.3
02:35:39.23 +57:45:01.8
01:38:33.81 +60:47:25.6
02:35:28.55 +57:41:15.0
02:24:51.53 +56:15:26.9
02:26:24.74 +56:14:06.4
02:19:14.48 +56:36:18.0
01:31:48.60 +64:22:28.2
01:49:47.70 +65:03:21.5
00:53:38.56 +65:00:02.2
01:39:32.69 +64:53:03.9
02:27:22.11 +62:38:26.1
02:02:57.28 +62:23:12.1
02:43:44.96 +60:25:27.3
01:27:44.41 +62:06:39.4
########### Completed Cas-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
01:56:38.09 +59:15:33.9
01:16:28.97 +60:14:00.3
02:24:29.85 +59:24:31.1
02:21:40.72 +60:54:41.9
02:28:33.48 +62:03:22.8
02:52:02.80 +63:39:30.2
01:59:42.41 +63:32:29.7
02:14:53.05 +64:11:56.5
02:08:06.43 +63:06:02.0
01:13:39.59 +63:12:31.2
01:00:19.87 +57:17:48.3
00:46:00.34 +57:56:20.1
00:37:39.91 +62:15:59.9
01:02:20.28 +57:02:48.2
01:08:39.11 +60:32:48.4
01:19:04.47 +60:02:34.1
00:47:54.55 +59:03:26.0
01:42:54.46 +61:13:30.6
02:52:09.97 +62:49:57.4
02:27:39.78 +57:06:42.3
02:30:58.90 +62:01:46.4
01:17:48.39 +57:17:35.2
01:57:25.08 +60:33:52.9
02:28:28.47 +58:25:05.6
02:37:12.84 +63:10:37.8
00:55:16.01 +57:59:06.5
00:56:47.59 +60:38:47.2
02:01:32.89 +65:05:48.8
01:59:56.21 +56:37:09.2
01:08:29.49 +57:06:54.4
00:52:55.06 +58:28:52.6
02:17:47.56 +56:14:45.2
02:36:02.71 +59:00:55.3
02:25:54.13 +56:38:48.5
02:18:52.86 +63:06:09.6
00:30:29.66 +66:05:42.3
02:19:40.58 +56:48:52.6
01:25:15.63 +64:40:33.5
00:46:11.73 +59:43:33.6
02:19:45.01 +56:50:30.5
02:20:35.00 +57:06:52.7
02:00:17.31 +65:03:54.9
02:20:50.58 +57:20:41.9
01:43:21.66 +56:52:28.8
00:36:54.99 +62:40:45.5
02:19:45.19 +57:01:14.5
02:29:09.04 +56:37:12.3
02:25:27.60 +56:46:56.1
02:34:10.54 +55:50:00.3
02:23:38.00 +56:52:44.8
02:22:03.76 +56:31:27.4
02:32:34.58 +57:29:15.3
02:34:00.78 +57:49:58.1
02:25:20.48 +56:51:13.6
02:29:10.13 +56:27:12.4
02:35:37.82 +57:29:13.2
02:27:24.37 +56:23:03.5
02:23:35.48 +56:34:27.4
02:34:44.20 +56:06:07.0
02:24:11.88 +56:35:43.2
02:33:34.76 +55:54:25.0
02:31:26.00 +55:59:07.0
02:18:01.26 +56:15:41.5
02:36:36.22 +57:46:58.9
02:19:46.68 +56:22:26.5
02:35:52.03 +57:47:22.2
02:23:26.41 +56:06:42.3
02:36:33.27 +57:54:38.9
02:21:55.20 +56:25:08.5
02:21:50.33 +56:34:31.6
02:20:54.08 +56:16:37.4
02:22:35.38 +56:18:13.9
02:34:44.93 +57:54:58.3
02:30:44.95 +56:56:12.6
02:32:05.73 +57:22:03.4
02:21:20.53 +56:29:12.7
02:24:43.66 +56:59:33.7
02:22:06.90 +56:07:52.9
02:37:36.88 +57:51:16.7
02:33:01.74 +57:02:07.9
02:19:52.93 +56:15:40.7
02:22:10.20 +56:24:23.3
02:19:48.61 +56:23:45.9
02:19:36.43 +56:14:20.7
02:27:48.55 +57:05:55.3
02:24:42.01 +56:55:47.8
02:32:45.26 +57:08:08.0
02:25:28.19 +56:11:20.2
02:25:20.40 +56:12:12.7
02:18:48.49 +56:17:54.8
02:23:42.88 +56:07:10.8
02:21:54.94 +56:42:38.7
02:20:55.04 +56:23:19.2
02:20:32.11 +56:10:00.6
02:27:07.72 +56:33:53.0
02:23:57.26 +57:12:24.5
02:31:12.06 +57:09:47.8
02:24:09.74 +56:34:02.3
02:22:04.60 +57:10:38.0
02:31:25.89 +56:07:05.1
02:32:04.83 +56:49:24.9
02:22:53.49 +56:47:13.1
02:33:49.40 +57:35:12.5
02:35:18.48 +57:31:39.8
02:30:51.91 +57:04:09.8
02:38:46.76 +57:49:57.1
02:25:33.89 +56:34:21.9
02:30:00.34 +57:28:19.7
02:28:50.69 +56:20:49.6
02:31:38.55 +57:13:46.4
02:36:35.03 +57:36:36.2
02:24:06.49 +56:29:59.8
02:24:33.46 +56:57:18.3
02:19:39.63 +56:20:11.8
02:29:17.13 +57:14:30.0
02:26:07.35 +56:25:11.7
02:21:55.92 +56:44:53.0
02:35:20.24 +57:29:29.9
02:19:45.17 +56:31:44.3
02:21:04.75 +56:15:32.3
02:30:33.01 +56:53:09.2
02:33:48.55 +57:01:45.9
02:31:18.70 +55:53:50.8
02:36:08.52 +57:39:33.9
02:30:32.25 +57:11:26.3
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02:31:12.57 +57:00:49.3
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00:36:55.91 +62:32:56.0
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02:29:25.87 +55:58:55.7
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02:26:20.11 +57:00:45.6
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02:34:35.60 +57:34:23.2
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02:32:54.63 +57:10:57.1
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02:23:18.87 +57:06:02.1
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02:20:23.58 +56:22:39.7
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02:25:05.47 +56:20:33.3
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02:32:01.41 +55:53:20.2
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02:23:29.57 +56:10:15.1
02:34:46.00 +58:00:26.7
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02:37:47.78 +57:52:43.0
02:24:54.07 +56:55:39.8
02:37:58.92 +58:07:38.9
02:27:22.03 +56:50:16.1
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02:20:13.03 +56:15:34.8
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02:30:08.47 +57:20:50.2
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02:22:07.92 +56:28:58.2
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02:27:20.09 +56:49:46.3
02:28:36.20 +56:28:40.0
02:23:45.93 +56:58:54.6
02:28:30.00 +56:31:48.6
02:28:30.82 +57:06:37.8
02:25:01.45 +56:33:15.8
02:30:19.39 +57:30:27.0
02:33:38.71 +57:12:31.9
02:32:02.17 +57:26:35.5
02:33:09.48 +57:50:43.7
02:24:54.81 +56:34:32.0
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02:31:40.18 +57:12:25.9
02:21:22.21 +56:42:51.2
02:32:03.60 +57:19:01.2
02:29:35.90 +56:47:29.8
00:45:31.36 +61:20:32.6
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02:25:03.41 +56:05:16.2
02:31:07.14 +56:54:53.9
02:29:01.50 +57:51:35.8
02:35:08.92 +57:20:11.7
02:38:11.28 +57:54:13.4
02:28:13.34 +57:23:00.9
01:31:48.44 +64:21:56.3
01:19:41.78 +62:51:03.2
02:37:45.34 +58:30:48.3
02:35:39.23 +57:45:01.8
01:38:33.81 +60:47:25.6
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02:19:14.48 +56:36:18.0
01:31:48.60 +64:22:28.2
02:32:01.89 +57:03:30.5
02:32:59.26 +57:53:54.0
02:38:06.09 +59:06:42.5
02:15:35.85 +56:21:36.3
02:38:02.06 +58:50:39.8
02:25:13.30 +56:30:31.2
02:05:05.77 +58:16:23.4
02:32:25.11 +58:26:07.8
02:33:34.78 +57:08:52.6
01:27:44.41 +62:06:39.4
01:41:47.10 +59:03:46.9
02:19:16.67 +59:42:21.1
01:39:32.69 +64:53:03.9
02:14:25.04 +56:42:47.8
02:20:07.53 +56:21:00.9
02:19:48.00 +56:25:10.7
02:34:13.06 +56:03:48.9
02:22:56.71 +57:11:44.4
02:25:27.49 +56:21:40.8
02:18:24.84 +58:37:26.7
02:23:49.27 +56:41:24.8
02:34:03.25 +56:00:34.3
01:49:47.70 +65:03:21.5
01:43:36.46 +58:48:08.2
02:38:48.34 +57:57:34.8
01:24:30.70 +59:38:48.0
02:27:22.11 +62:38:26.1
02:21:26.42 +57:16:57.3
02:27:55.31 +56:27:24.0
02:43:44.96 +60:25:27.3
02:33:40.23 +57:40:02.3
02:17:25.67 +57:06:42.6
02:37:50.78 +57:54:15.9
02:32:22.33 +58:28:54.9
02:21:36.06 +57:03:37.7
01:33:44.53 +60:46:20.5
00:53:38.56 +65:00:02.2
02:02:57.28 +62:23:12.1
02:31:45.85 +55:57:57.7
02:17:01.95 +56:44:19.3
01:52:19.58 +57:19:07.2
02:49:56.76 +63:51:39.5
02:29:48.78 +57:57:50.6
02:31:31.28 +57:22:45.9
01:43:45.33 +58:23:44.8
###################################################################################
01:56:38.09 +59:15:33.9 -- not an asteroid (will add it to exclusion list)
01:16:28.97 +60:14:00.3 -- not an asteroid (will add it to exclusion list)
02:24:29.85 +59:24:31.1 -- not an asteroid (will add it to exclusion list)
02:21:40.72 +60:54:41.9 -- not an asteroid (will add it to exclusion list)
02:28:33.48 +62:03:22.8 -- not an asteroid (will add it to exclusion list)
02:52:02.80 +63:39:30.2 -- not an asteroid (will add it to exclusion list)
01:59:42.41 +63:32:29.7 -- not an asteroid (will add it to exclusion list)
02:14:53.05 +64:11:56.5 -- not an asteroid (will add it to exclusion list)
02:08:06.43 +63:06:02.0 -- not an asteroid (will add it to exclusion list)
01:13:39.59 +63:12:31.2 -- not an asteroid (will add it to exclusion list)
01:00:19.87 +57:17:48.3 -- not an asteroid (will add it to exclusion list)
00:46:00.34 +57:56:20.1 -- not an asteroid (will add it to exclusion list)
00:37:39.91 +62:15:59.9 -- not an asteroid (will add it to exclusion list)
01:02:20.28 +57:02:48.2 -- not an asteroid (will add it to exclusion list)
01:08:39.11 +60:32:48.4 -- not an asteroid (will add it to exclusion list)
01:19:04.47 +60:02:34.1 -- not an asteroid (will add it to exclusion list)
00:47:54.55 +59:03:26.0 -- not an asteroid (will add it to exclusion list)
01:42:54.46 +61:13:30.6 -- not an asteroid (will add it to exclusion list)
02:52:09.97 +62:49:57.4 -- not an asteroid (will add it to exclusion list)
02:27:39.78 +57:06:42.3 -- not an asteroid (will add it to exclusion list)
02:30:58.90 +62:01:46.4 -- not an asteroid (will add it to exclusion list)
01:17:48.39 +57:17:35.2 -- not an asteroid (will add it to exclusion list)
01:57:25.08 +60:33:52.9 -- not an asteroid (will add it to exclusion list)
02:28:28.47 +58:25:05.6 -- not an asteroid (will add it to exclusion list)
02:37:12.84 +63:10:37.8 -- not an asteroid (will add it to exclusion list)
00:55:16.01 +57:59:06.5 -- not an asteroid (will add it to exclusion list)
00:56:47.59 +60:38:47.2 -- not an asteroid (will add it to exclusion list)
02:01:32.89 +65:05:48.8 -- not an asteroid (will add it to exclusion list)
01:59:56.21 +56:37:09.2 -- not an asteroid (will add it to exclusion list)
01:08:29.49 +57:06:54.4 -- not an asteroid (will add it to exclusion list)
00:52:55.06 +58:28:52.6 -- not an asteroid (will add it to exclusion list)
02:17:47.56 +56:14:45.2 -- not an asteroid (will add it to exclusion list)
02:36:02.71 +59:00:55.3 -- not an asteroid (will add it to exclusion list)
02:25:54.13 +56:38:48.5 -- not an asteroid (will add it to exclusion list)
02:18:52.86 +63:06:09.6 -- not an asteroid (will add it to exclusion list)
00:30:29.66 +66:05:42.3 -- not an asteroid (will add it to exclusion list)
02:19:40.58 +56:48:52.6 -- not an asteroid (will add it to exclusion list)
01:25:15.63 +64:40:33.5 -- not an asteroid (will add it to exclusion list)
00:46:11.73 +59:43:33.6 -- not an asteroid (will add it to exclusion list)
02:19:45.01 +56:50:30.5 -- not an asteroid (will add it to exclusion list)
02:20:35.00 +57:06:52.7 -- not an asteroid (will add it to exclusion list)
02:00:17.31 +65:03:54.9 -- not an asteroid (will add it to exclusion list)
02:20:50.58 +57:20:41.9 -- not an asteroid (will add it to exclusion list)
01:43:21.66 +56:52:28.8 -- not an asteroid (will add it to exclusion list)
00:36:54.99 +62:40:45.5 -- not an asteroid (will add it to exclusion list)
02:19:45.19 +57:01:14.5 -- not an asteroid (will add it to exclusion list)
02:29:09.04 +56:37:12.3 -- not an asteroid (will add it to exclusion list)
02:25:27.60 +56:46:56.1 -- not an asteroid (will add it to exclusion list)
02:34:10.54 +55:50:00.3 -- not an asteroid (will add it to exclusion list)
02:23:38.00 +56:52:44.8 -- not an asteroid (will add it to exclusion list)
02:22:03.76 +56:31:27.4 -- not an asteroid (will add it to exclusion list)
02:32:34.58 +57:29:15.3 -- not an asteroid (will add it to exclusion list)
02:34:00.78 +57:49:58.1 -- not an asteroid (will add it to exclusion list)
02:25:20.48 +56:51:13.6 -- not an asteroid (will add it to exclusion list)
02:29:10.13 +56:27:12.4 -- not an asteroid (will add it to exclusion list)
02:35:37.82 +57:29:13.2 -- not an asteroid (will add it to exclusion list)
02:27:24.37 +56:23:03.5 -- not an asteroid (will add it to exclusion list)
02:23:35.48 +56:34:27.4 -- not an asteroid (will add it to exclusion list)
02:34:44.20 +56:06:07.0 -- not an asteroid (will add it to exclusion list)
02:24:11.88 +56:35:43.2 -- not an asteroid (will add it to exclusion list)
02:33:34.76 +55:54:25.0 -- not an asteroid (will add it to exclusion list)
02:31:26.00 +55:59:07.0 -- not an asteroid (will add it to exclusion list)
02:18:01.26 +56:15:41.5 -- not an asteroid (will add it to exclusion list)
02:36:36.22 +57:46:58.9 -- not an asteroid (will add it to exclusion list)
02:19:46.68 +56:22:26.5 -- not an asteroid (will add it to exclusion list)
02:35:52.03 +57:47:22.2 -- not an asteroid (will add it to exclusion list)
02:23:26.41 +56:06:42.3 -- not an asteroid (will add it to exclusion list)
02:36:33.27 +57:54:38.9 -- not an asteroid (will add it to exclusion list)
02:21:55.20 +56:25:08.5 -- not an asteroid (will add it to exclusion list)
02:21:50.33 +56:34:31.6 -- not an asteroid (will add it to exclusion list)
02:20:54.08 +56:16:37.4 -- not an asteroid (will add it to exclusion list)
02:22:35.38 +56:18:13.9 -- not an asteroid (will add it to exclusion list)
02:34:44.93 +57:54:58.3 -- not an asteroid (will add it to exclusion list)
02:30:44.95 +56:56:12.6 -- not an asteroid (will add it to exclusion list)
02:32:05.73 +57:22:03.4 -- not an asteroid (will add it to exclusion list)
02:21:20.53 +56:29:12.7 -- not an asteroid (will add it to exclusion list)
02:24:43.66 +56:59:33.7 -- not an asteroid (will add it to exclusion list)
02:22:06.90 +56:07:52.9 -- not an asteroid (will add it to exclusion list)
02:37:36.88 +57:51:16.7 -- not an asteroid (will add it to exclusion list)
02:33:01.74 +57:02:07.9 -- not an asteroid (will add it to exclusion list)
02:19:52.93 +56:15:40.7 -- not an asteroid (will add it to exclusion list)
02:22:10.20 +56:24:23.3 -- not an asteroid (will add it to exclusion list)
02:19:48.61 +56:23:45.9 -- not an asteroid (will add it to exclusion list)
02:19:36.43 +56:14:20.7 -- not an asteroid (will add it to exclusion list)
02:27:48.55 +57:05:55.3 -- not an asteroid (will add it to exclusion list)
02:24:42.01 +56:55:47.8 -- not an asteroid (will add it to exclusion list)
02:32:45.26 +57:08:08.0 -- not an asteroid (will add it to exclusion list)
02:25:28.19 +56:11:20.2 -- not an asteroid (will add it to exclusion list)
02:25:20.40 +56:12:12.7 -- not an asteroid (will add it to exclusion list)
02:18:48.49 +56:17:54.8 -- not an asteroid (will add it to exclusion list)
02:23:42.88 +56:07:10.8 -- not an asteroid (will add it to exclusion list)
02:21:54.94 +56:42:38.7 -- not an asteroid (will add it to exclusion list)
02:20:55.04 +56:23:19.2 -- not an asteroid (will add it to exclusion list)
02:20:32.11 +56:10:00.6 -- not an asteroid (will add it to exclusion list)
02:27:07.72 +56:33:53.0 -- not an asteroid (will add it to exclusion list)
02:23:57.26 +57:12:24.5 -- not an asteroid (will add it to exclusion list)
02:31:12.06 +57:09:47.8 -- not an asteroid (will add it to exclusion list)
02:24:09.74 +56:34:02.3 -- not an asteroid (will add it to exclusion list)
02:22:04.60 +57:10:38.0 -- not an asteroid (will add it to exclusion list)
02:31:25.89 +56:07:05.1 -- not an asteroid (will add it to exclusion list)
02:32:04.83 +56:49:24.9 -- not an asteroid (will add it to exclusion list)
02:22:53.49 +56:47:13.1 -- not an asteroid (will add it to exclusion list)
02:33:49.40 +57:35:12.5 -- not an asteroid (will add it to exclusion list)
02:35:18.48 +57:31:39.8 -- not an asteroid (will add it to exclusion list)
02:30:51.91 +57:04:09.8 -- not an asteroid (will add it to exclusion list)
02:38:46.76 +57:49:57.1 -- not an asteroid (will add it to exclusion list)
02:25:33.89 +56:34:21.9 -- not an asteroid (will add it to exclusion list)
02:30:00.34 +57:28:19.7 -- not an asteroid (will add it to exclusion list)
02:28:50.69 +56:20:49.6 -- not an asteroid (will add it to exclusion list)
02:31:38.55 +57:13:46.4 -- not an asteroid (will add it to exclusion list)
02:36:35.03 +57:36:36.2 -- not an asteroid (will add it to exclusion list)
02:24:06.49 +56:29:59.8 -- not an asteroid (will add it to exclusion list)
02:24:33.46 +56:57:18.3 -- not an asteroid (will add it to exclusion list)
02:19:39.63 +56:20:11.8 -- not an asteroid (will add it to exclusion list)
02:29:17.13 +57:14:30.0 -- not an asteroid (will add it to exclusion list)
02:26:07.35 +56:25:11.7 -- not an asteroid (will add it to exclusion list)
02:21:55.92 +56:44:53.0 -- not an asteroid (will add it to exclusion list)
02:35:20.24 +57:29:29.9 -- not an asteroid (will add it to exclusion list)
02:19:45.17 +56:31:44.3 -- not an asteroid (will add it to exclusion list)
02:21:04.75 +56:15:32.3 -- not an asteroid (will add it to exclusion list)
02:30:33.01 +56:53:09.2 -- not an asteroid (will add it to exclusion list)
02:33:48.55 +57:01:45.9 -- not an asteroid (will add it to exclusion list)
02:31:18.70 +55:53:50.8 -- not an asteroid (will add it to exclusion list)
02:36:08.52 +57:39:33.9 -- not an asteroid (will add it to exclusion list)
02:30:32.25 +57:11:26.3 -- not an asteroid (will add it to exclusion list)
02:21:59.09 +56:30:01.6 -- not an asteroid (will add it to exclusion list)
02:25:03.15 +56:56:58.8 -- not an asteroid (will add it to exclusion list)
02:22:31.56 +56:14:10.7 -- not an asteroid (will add it to exclusion list)
02:24:18.81 +56:54:02.0 -- not an asteroid (will add it to exclusion list)
02:25:00.78 +56:51:31.9 -- not an asteroid (will add it to exclusion list)
02:19:56.52 +56:13:26.0 -- not an asteroid (will add it to exclusion list)
02:26:13.46 +56:36:46.9 -- not an asteroid (will add it to exclusion list)
02:27:33.11 +56:13:09.8 -- not an asteroid (will add it to exclusion list)
02:29:26.34 +57:23:02.8 -- not an asteroid (will add it to exclusion list)
02:23:02.19 +56:30:28.6 -- not an asteroid (will add it to exclusion list)
02:31:20.24 +57:33:46.4 -- not an asteroid (will add it to exclusion list)
02:24:32.63 +57:00:44.1 -- not an asteroid (will add it to exclusion list)
02:29:28.55 +56:33:06.0 -- not an asteroid (will add it to exclusion list)
02:16:52.43 +56:18:43.8 -- not an asteroid (will add it to exclusion list)
02:18:24.03 +56:23:21.4 -- not an asteroid (will add it to exclusion list)
02:26:55.75 +56:30:20.2 -- not an asteroid (will add it to exclusion list)
02:30:30.83 +57:30:27.8 -- not an asteroid (will add it to exclusion list)
02:23:48.03 +56:47:01.5 -- not an asteroid (will add it to exclusion list)
02:26:10.79 +56:48:28.8 -- not an asteroid (will add it to exclusion list)
02:33:09.10 +57:00:38.5 -- not an asteroid (will add it to exclusion list)
02:33:40.71 +57:26:09.7 -- not an asteroid (will add it to exclusion list)
02:36:22.58 +57:40:05.6 -- not an asteroid (will add it to exclusion list)
02:25:48.44 +56:55:12.4 -- not an asteroid (will add it to exclusion list)
02:23:17.91 +56:42:23.9 -- not an asteroid (will add it to exclusion list)
02:20:18.71 +56:31:49.5 -- not an asteroid (will add it to exclusion list)
02:21:34.57 +56:26:43.9 -- not an asteroid (will add it to exclusion list)
02:19:36.20 +56:23:21.9 -- not an asteroid (will add it to exclusion list)
02:25:56.01 +56:58:59.2 -- not an asteroid (will add it to exclusion list)
02:35:08.67 +57:36:14.5 -- not an asteroid (will add it to exclusion list)
02:37:50.64 +57:45:49.7 -- not an asteroid (will add it to exclusion list)
02:26:43.23 +56:24:12.4 -- not an asteroid (will add it to exclusion list)
02:35:04.64 +57:26:52.9 -- not an asteroid (will add it to exclusion list)
02:24:34.14 +56:53:00.2 -- not an asteroid (will add it to exclusion list)
02:22:27.95 +56:41:51.9 -- not an asteroid (will add it to exclusion list)
02:26:11.70 +56:56:03.6 -- not an asteroid (will add it to exclusion list)
02:18:05.24 +56:15:07.5 -- not an asteroid (will add it to exclusion list)
02:34:48.66 +57:38:04.9 -- not an asteroid (will add it to exclusion list)
02:27:59.53 +56:29:42.2 -- not an asteroid (will add it to exclusion list)
02:29:33.00 +55:57:16.1 -- not an asteroid (will add it to exclusion list)
02:24:02.04 +56:49:22.3 -- not an asteroid (will add it to exclusion list)
02:23:55.73 +56:44:45.5 -- not an asteroid (will add it to exclusion list)
02:21:52.12 +56:41:17.7 -- not an asteroid (will add it to exclusion list)
02:32:17.85 +57:17:09.3 -- not an asteroid (will add it to exclusion list)
02:23:38.21 +56:39:53.8 -- not an asteroid (will add it to exclusion list)
02:31:29.32 +57:11:54.7 -- not an asteroid (will add it to exclusion list)
02:37:50.68 +57:57:56.9 -- not an asteroid (will add it to exclusion list)
02:21:30.49 +57:12:34.5 -- not an asteroid (will add it to exclusion list)
02:25:30.12 +56:16:52.8 -- not an asteroid (will add it to exclusion list)
02:31:09.75 +57:16:14.4 -- not an asteroid (will add it to exclusion list)
02:20:07.36 +56:27:52.1 -- not an asteroid (will add it to exclusion list)
02:33:34.12 +55:49:25.9 -- not an asteroid (will add it to exclusion list)
02:33:03.26 +57:03:29.0 -- not an asteroid (will add it to exclusion list)
02:33:10.59 +57:32:53.7 -- not an asteroid (will add it to exclusion list)
02:36:59.45 +57:56:29.8 -- not an asteroid (will add it to exclusion list)
02:32:14.18 +55:56:22.8 -- not an asteroid (will add it to exclusion list)
02:25:56.75 +56:07:50.5 -- not an asteroid (will add it to exclusion list)
02:25:04.29 +56:13:07.5 -- not an asteroid (will add it to exclusion list)
02:33:34.41 +56:11:48.0 -- not an asteroid (will add it to exclusion list)
02:34:24.39 +57:28:26.1 -- not an asteroid (will add it to exclusion list)
02:38:13.42 +57:50:16.2 -- not an asteroid (will add it to exclusion list)
02:28:48.05 +56:30:07.8 -- not an asteroid (will add it to exclusion list)
02:33:54.63 +57:40:55.2 -- not an asteroid (will add it to exclusion list)
02:25:42.31 +56:37:12.9 -- not an asteroid (will add it to exclusion list)
02:21:55.06 +56:20:50.1 -- not an asteroid (will add it to exclusion list)
02:24:25.89 +56:32:55.3 -- not an asteroid (will add it to exclusion list)
02:24:47.99 +56:36:57.6 -- not an asteroid (will add it to exclusion list)
02:24:32.13 +56:43:35.2 -- not an asteroid (will add it to exclusion list)
02:26:15.82 +56:04:34.0 -- not an asteroid (will add it to exclusion list)
02:25:45.49 +56:26:32.2 -- not an asteroid (will add it to exclusion list)
02:21:36.86 +56:40:52.1 -- not an asteroid (will add it to exclusion list)
02:30:39.48 +57:13:42.2 -- not an asteroid (will add it to exclusion list)
02:25:07.44 +56:14:04.5 -- not an asteroid (will add it to exclusion list)
02:26:00.84 +56:46:18.0 -- not an asteroid (will add it to exclusion list)
02:26:59.49 +57:14:44.2 -- not an asteroid (will add it to exclusion list)
02:31:10.54 +57:30:46.6 -- not an asteroid (will add it to exclusion list)
02:29:57.33 +56:36:50.4 -- not an asteroid (will add it to exclusion list)
02:31:12.57 +57:00:49.3 -- not an asteroid (will add it to exclusion list)
02:20:24.56 +56:41:43.6 -- not an asteroid (will add it to exclusion list)
02:23:44.10 +56:55:56.9 -- not an asteroid (will add it to exclusion list)
02:23:14.27 +56:52:06.4 -- not an asteroid (will add it to exclusion list)
02:26:08.97 +56:16:06.3 -- not an asteroid (will add it to exclusion list)
02:33:43.78 +57:36:02.2 -- not an asteroid (will add it to exclusion list)
02:37:02.20 +57:41:39.3 -- not an asteroid (will add it to exclusion list)
02:33:51.00 +55:59:56.1 -- not an asteroid (will add it to exclusion list)
02:30:11.98 +57:38:18.7 -- not an asteroid (will add it to exclusion list)
02:21:27.44 +56:16:28.6 -- not an asteroid (will add it to exclusion list)
01:40:01.08 +60:52:38.4 -- not an asteroid (will add it to exclusion list)
02:26:02.37 +56:20:59.5 -- not an asteroid (will add it to exclusion list)
02:24:23.74 +56:54:04.6 -- not an asteroid (will add it to exclusion list)
02:24:38.20 +56:49:55.7 -- not an asteroid (will add it to exclusion list)
02:27:52.28 +56:29:28.8 -- not an asteroid (will add it to exclusion list)
02:25:32.87 +56:32:57.7 -- not an asteroid (will add it to exclusion list)
02:22:11.95 +56:20:47.3 -- not an asteroid (will add it to exclusion list)
02:33:49.02 +55:57:06.8 -- not an asteroid (will add it to exclusion list)
02:31:19.72 +56:52:39.5 -- not an asteroid (will add it to exclusion list)
02:30:19.30 +55:54:55.0 -- not an asteroid (will add it to exclusion list)
02:31:00.30 +56:00:28.1 -- not an asteroid (will add it to exclusion list)
02:25:11.80 +56:17:22.8 -- not an asteroid (will add it to exclusion list)
02:24:18.84 +56:19:49.3 -- not an asteroid (will add it to exclusion list)
02:25:48.43 +56:32:35.4 -- not an asteroid (will add it to exclusion list)
02:32:04.94 +56:53:51.4 -- not an asteroid (will add it to exclusion list)
02:32:35.29 +57:32:20.9 -- not an asteroid (will add it to exclusion list)
02:30:45.41 +57:06:28.3 -- not an asteroid (will add it to exclusion list)
02:35:26.60 +57:46:11.7 -- not an asteroid (will add it to exclusion list)
02:23:07.47 +56:41:44.4 -- not an asteroid (will add it to exclusion list)
02:30:51.81 +57:15:44.6 -- not an asteroid (will add it to exclusion list)
02:23:08.48 +56:20:24.9 -- not an asteroid (will add it to exclusion list)
02:30:16.92 +56:38:09.4 -- not an asteroid (will add it to exclusion list)
02:24:52.38 +56:43:10.9 -- not an asteroid (will add it to exclusion list)
02:35:34.92 +57:32:59.3 -- not an asteroid (will add it to exclusion list)
02:28:32.01 +56:00:36.5 -- not an asteroid (will add it to exclusion list)
02:24:53.93 +56:08:45.2 -- not an asteroid (will add it to exclusion list)
02:27:34.40 +56:16:53.2 -- not an asteroid (will add it to exclusion list)
02:36:55.81 +57:38:49.8 -- not an asteroid (will add it to exclusion list)
02:34:12.97 +56:11:54.0 -- not an asteroid (will add it to exclusion list)
02:20:11.71 +56:22:22.8 -- not an asteroid (will add it to exclusion list)
02:29:55.64 +56:55:49.6 -- not an asteroid (will add it to exclusion list)
02:30:33.48 +56:57:02.6 -- not an asteroid (will add it to exclusion list)
02:31:03.43 +55:52:01.6 -- not an asteroid (will add it to exclusion list)
02:20:25.25 +56:52:28.8 -- not an asteroid (will add it to exclusion list)
02:23:11.37 +56:11:21.3 -- not an asteroid (will add it to exclusion list)
02:26:55.66 +56:28:24.5 -- not an asteroid (will add it to exclusion list)
02:22:16.04 +56:22:42.6 -- not an asteroid (will add it to exclusion list)
02:27:23.12 +56:19:27.5 -- not an asteroid (will add it to exclusion list)
02:33:27.67 +57:14:45.0 -- not an asteroid (will add it to exclusion list)
02:24:46.87 +56:38:55.3 -- not an asteroid (will add it to exclusion list)
02:29:39.11 +56:11:33.0 -- not an asteroid (will add it to exclusion list)
02:37:01.15 +57:51:23.0 -- not an asteroid (will add it to exclusion list)
02:32:23.31 +57:38:37.3 -- not an asteroid (will add it to exclusion list)
02:24:38.57 +56:20:45.4 -- not an asteroid (will add it to exclusion list)
02:30:35.00 +56:43:58.4 -- not an asteroid (will add it to exclusion list)
02:31:51.45 +56:45:51.1 -- not an asteroid (will add it to exclusion list)
02:32:55.48 +57:08:54.0 -- not an asteroid (will add it to exclusion list)
02:34:13.94 +56:18:42.0 -- not an asteroid (will add it to exclusion list)
02:29:11.28 +57:21:01.0 -- not an asteroid (will add it to exclusion list)
02:27:53.71 +57:06:30.9 -- not an asteroid (will add it to exclusion list)
02:32:01.27 +56:51:17.5 -- not an asteroid (will add it to exclusion list)
02:33:37.69 +57:40:25.1 -- not an asteroid (will add it to exclusion list)
00:43:47.78 +61:53:59.7 -- not an asteroid (will add it to exclusion list)
02:32:47.65 +57:14:17.2 -- not an asteroid (will add it to exclusion list)
02:22:21.43 +56:34:19.1 -- not an asteroid (will add it to exclusion list)
02:32:49.40 +57:34:21.9 -- not an asteroid (will add it to exclusion list)
02:20:54.28 +56:36:05.4 -- not an asteroid (will add it to exclusion list)
02:22:22.77 +56:40:00.7 -- not an asteroid (will add it to exclusion list)
02:27:27.07 +56:31:10.2 -- not an asteroid (will add it to exclusion list)
02:21:52.46 +56:32:45.3 -- not an asteroid (will add it to exclusion list)
02:24:12.53 +56:49:25.8 -- not an asteroid (will add it to exclusion list)
02:21:33.10 +56:13:41.1 -- not an asteroid (will add it to exclusion list)
02:25:40.03 +56:29:20.6 -- not an asteroid (will add it to exclusion list)
02:21:38.53 +56:26:50.2 -- not an asteroid (will add it to exclusion list)
02:26:14.40 +56:12:13.5 -- not an asteroid (will add it to exclusion list)
02:39:23.99 +58:09:11.5 -- not an asteroid (will add it to exclusion list)
02:36:41.37 +57:37:08.5 -- not an asteroid (will add it to exclusion list)
02:35:58.35 +57:49:15.3 -- not an asteroid (will add it to exclusion list)
02:39:21.42 +58:07:09.8 -- not an asteroid (will add it to exclusion list)
02:29:41.54 +56:37:30.7 -- not an asteroid (will add it to exclusion list)
00:58:55.93 +58:04:05.2 -- not an asteroid (will add it to exclusion list)
02:33:30.94 +57:29:02.8 -- not an asteroid (will add it to exclusion list)
02:22:47.76 +56:11:09.8 -- not an asteroid (will add it to exclusion list)
02:21:19.11 +56:38:13.4 -- not an asteroid (will add it to exclusion list)
02:17:41.08 +56:28:32.5 -- not an asteroid (will add it to exclusion list)
02:28:01.17 +56:23:28.1 -- not an asteroid (will add it to exclusion list)
02:21:16.36 +56:23:43.0 -- not an asteroid (will add it to exclusion list)
02:24:58.44 +56:50:40.4 -- not an asteroid (will add it to exclusion list)
02:25:52.54 +57:02:04.3 -- not an asteroid (will add it to exclusion list)
02:27:42.18 +56:12:19.8 -- not an asteroid (will add it to exclusion list)
02:23:54.58 +56:06:52.8 -- not an asteroid (will add it to exclusion list)
01:58:16.63 +59:38:57.1 -- not an asteroid (will add it to exclusion list)
02:31:45.84 +57:14:33.1 -- not an asteroid (will add it to exclusion list)
02:17:50.40 +56:22:37.9 -- not an asteroid (will add it to exclusion list)
02:21:13.54 +56:28:44.7 -- not an asteroid (will add it to exclusion list)
02:24:21.26 +56:52:14.7 -- not an asteroid (will add it to exclusion list)
02:24:38.41 +56:48:43.1 -- not an asteroid (will add it to exclusion list)
02:34:31.90 +57:40:30.4 -- not an asteroid (will add it to exclusion list)
02:26:01.02 +56:28:14.9 -- not an asteroid (will add it to exclusion list)
02:23:57.17 +56:11:53.7 -- not an asteroid (will add it to exclusion list)
01:29:32.95 +61:46:25.0 -- not an asteroid (will add it to exclusion list)
02:34:04.49 +57:32:44.3 -- not an asteroid (will add it to exclusion list)
02:36:12.26 +57:41:56.0 -- not an asteroid (will add it to exclusion list)
02:28:09.05 +56:38:21.2 -- not an asteroid (will add it to exclusion list)
01:18:14.29 +61:44:36.0 -- not an asteroid (will add it to exclusion list)
02:31:47.11 +55:52:28.5 -- not an asteroid (will add it to exclusion list)
02:27:22.05 +56:31:18.8 -- not an asteroid (will add it to exclusion list)
02:37:15.58 +57:48:19.2 -- not an asteroid (will add it to exclusion list)
02:21:39.29 +56:31:44.8 -- not an asteroid (will add it to exclusion list)
02:33:11.11 +57:33:48.8 -- not an asteroid (will add it to exclusion list)
02:23:43.00 +56:38:37.8 -- not an asteroid (will add it to exclusion list)
02:20:52.81 +56:09:33.8 -- not an asteroid (will add it to exclusion list)
02:34:19.87 +57:08:33.3 -- not an asteroid (will add it to exclusion list)
00:36:55.91 +62:32:56.0 -- not an asteroid (will add it to exclusion list)
02:30:17.43 +56:43:02.2 -- not an asteroid (will add it to exclusion list)
02:28:44.08 +57:00:25.5 -- not an asteroid (will add it to exclusion list)
02:31:18.74 +57:03:50.9 -- not an asteroid (will add it to exclusion list)
02:18:56.21 +56:18:32.0 -- not an asteroid (will add it to exclusion list)
02:29:08.36 +57:12:16.0 -- not an asteroid (will add it to exclusion list)
02:23:53.85 +56:39:14.7 -- not an asteroid (will add it to exclusion list)
02:30:51.42 +57:16:48.8 -- not an asteroid (will add it to exclusion list)
02:35:42.02 +57:31:40.9 -- not an asteroid (will add it to exclusion list)
02:31:56.68 +57:24:00.2 -- not an asteroid (will add it to exclusion list)
02:38:19.87 +58:03:56.7 -- not an asteroid (will add it to exclusion list)
02:25:52.96 +56:47:30.0 -- not an asteroid (will add it to exclusion list)
02:33:08.29 +57:28:10.5 -- not an asteroid (will add it to exclusion list)
02:34:46.52 +57:13:22.5 -- not an asteroid (will add it to exclusion list)
02:30:07.17 +56:30:20.8 -- not an asteroid (will add it to exclusion list)
02:29:48.78 +56:41:55.8 -- not an asteroid (will add it to exclusion list)
02:26:58.18 +56:22:12.1 -- not an asteroid (will add it to exclusion list)
02:33:44.27 +56:59:34.7 -- not an asteroid (will add it to exclusion list)
02:33:03.94 +57:33:09.8 -- not an asteroid (will add it to exclusion list)
02:23:07.87 +56:29:01.2 -- not an asteroid (will add it to exclusion list)
02:25:56.53 +56:32:31.9 -- not an asteroid (will add it to exclusion list)
02:35:58.93 +57:32:00.1 -- not an asteroid (will add it to exclusion list)
02:27:44.66 +56:19:43.0 -- not an asteroid (will add it to exclusion list)
02:25:56.42 +57:04:40.2 -- not an asteroid (will add it to exclusion list)
02:31:02.85 +57:42:08.9 -- not an asteroid (will add it to exclusion list)
02:29:25.87 +55:58:55.7 -- not an asteroid (will add it to exclusion list)
02:31:52.57 +56:53:49.0 -- not an asteroid (will add it to exclusion list)
02:39:52.21 +58:24:37.9 -- not an asteroid (will add it to exclusion list)
02:27:18.72 +56:15:53.5 -- not an asteroid (will add it to exclusion list)
02:36:25.89 +57:52:58.9 -- not an asteroid (will add it to exclusion list)
02:24:27.20 +56:50:28.9 -- not an asteroid (will add it to exclusion list)
02:34:31.90 +56:11:08.8 -- not an asteroid (will add it to exclusion list)
02:27:31.55 +56:30:00.3 -- not an asteroid (will add it to exclusion list)
02:25:53.52 +56:14:35.6 -- not an asteroid (will add it to exclusion list)
02:30:58.33 +57:16:17.2 -- not an asteroid (will add it to exclusion list)
02:22:27.17 +56:43:56.9 -- not an asteroid (will add it to exclusion list)
02:24:37.23 +56:45:53.9 -- not an asteroid (will add it to exclusion list)
02:29:46.73 +56:03:52.6 -- not an asteroid (will add it to exclusion list)
02:24:29.35 +56:34:20.6 -- not an asteroid (will add it to exclusion list)
02:31:18.77 +57:16:22.0 -- not an asteroid (will add it to exclusion list)
02:31:20.63 +56:50:06.3 -- not an asteroid (will add it to exclusion list)
02:31:33.36 +57:25:43.5 -- not an asteroid (will add it to exclusion list)
02:21:07.65 +56:13:22.2 -- not an asteroid (will add it to exclusion list)
02:30:09.68 +57:23:15.1 -- not an asteroid (will add it to exclusion list)
02:33:18.10 +57:31:36.8 -- not an asteroid (will add it to exclusion list)
02:36:07.79 +57:32:58.9 -- not an asteroid (will add it to exclusion list)
02:34:41.26 +56:11:01.6 -- not an asteroid (will add it to exclusion list)
02:26:20.11 +57:00:45.6 -- not an asteroid (will add it to exclusion list)
02:30:53.15 +56:59:21.2 -- not an asteroid (will add it to exclusion list)
02:34:42.72 +57:17:58.8 -- not an asteroid (will add it to exclusion list)
02:27:57.88 +56:22:23.8 -- not an asteroid (will add it to exclusion list)
02:33:08.50 +57:21:20.2 -- not an asteroid (will add it to exclusion list)
02:37:52.11 +57:47:13.1 -- not an asteroid (will add it to exclusion list)
02:25:45.87 +56:22:47.0 -- not an asteroid (will add it to exclusion list)
02:38:14.42 +57:58:50.6 -- not an asteroid (will add it to exclusion list)
02:33:33.71 +57:37:46.7 -- not an asteroid (will add it to exclusion list)
02:21:35.29 +56:14:56.5 -- not an asteroid (will add it to exclusion list)
02:30:03.83 +56:36:39.2 -- not an asteroid (will add it to exclusion list)
02:26:36.42 +56:34:16.7 -- not an asteroid (will add it to exclusion list)
02:32:24.99 +57:27:18.3 -- not an asteroid (will add it to exclusion list)
02:29:29.43 +57:10:39.0 -- not an asteroid (will add it to exclusion list)
02:27:40.70 +56:20:28.5 -- not an asteroid (will add it to exclusion list)
02:34:04.61 +57:19:27.3 -- not an asteroid (will add it to exclusion list)
02:26:10.21 +56:21:10.3 -- not an asteroid (will add it to exclusion list)
02:22:29.14 +56:32:00.5 -- not an asteroid (will add it to exclusion list)
02:34:35.60 +57:34:23.2 -- not an asteroid (will add it to exclusion list)
02:34:46.10 +57:12:52.3 -- not an asteroid (will add it to exclusion list)
02:34:38.93 +57:26:15.3 -- not an asteroid (will add it to exclusion list)
02:32:54.63 +57:10:57.1 -- not an asteroid (will add it to exclusion list)
02:22:37.79 +56:37:17.0 -- not an asteroid (will add it to exclusion list)
02:23:18.87 +57:06:02.1 -- not an asteroid (will add it to exclusion list)
02:24:23.45 +56:13:56.3 -- not an asteroid (will add it to exclusion list)
02:20:23.58 +56:22:39.7 -- not an asteroid (will add it to exclusion list)
02:26:45.86 +56:23:26.2 -- not an asteroid (will add it to exclusion list)
02:30:55.12 +57:08:07.5 -- not an asteroid (will add it to exclusion list)
02:32:06.03 +57:05:00.6 -- not an asteroid (will add it to exclusion list)
02:25:39.55 +56:48:00.4 -- not an asteroid (will add it to exclusion list)
02:22:51.67 +56:24:33.0 -- not an asteroid (will add it to exclusion list)
02:25:12.20 +56:44:30.7 -- not an asteroid (will add it to exclusion list)
02:25:05.47 +56:20:33.3 -- not an asteroid (will add it to exclusion list)
02:25:48.30 +56:35:16.7 -- not an asteroid (will add it to exclusion list)
02:25:01.82 +56:15:07.5 -- not an asteroid (will add it to exclusion list)
02:32:01.41 +55:53:20.2 -- not an asteroid (will add it to exclusion list)
02:35:41.37 +57:27:01.8 -- not an asteroid (will add it to exclusion list)
02:24:54.82 +56:45:04.1 -- not an asteroid (will add it to exclusion list)
02:23:46.82 +57:05:04.4 -- not an asteroid (will add it to exclusion list)
02:27:24.28 +56:17:59.4 -- not an asteroid (will add it to exclusion list)
02:23:29.57 +56:10:15.1 -- not an asteroid (will add it to exclusion list)
02:34:46.00 +58:00:26.7 -- not an asteroid (will add it to exclusion list)
02:32:58.19 +57:38:43.0 -- not an asteroid (will add it to exclusion list)
02:37:47.78 +57:52:43.0 -- not an asteroid (will add it to exclusion list)
02:24:54.07 +56:55:39.8 -- not an asteroid (will add it to exclusion list)
02:37:58.92 +58:07:38.9 -- not an asteroid (will add it to exclusion list)
02:27:22.03 +56:50:16.1 -- not an asteroid (will add it to exclusion list)
02:36:17.73 +57:48:52.1 -- not an asteroid (will add it to exclusion list)
02:25:54.98 +56:55:26.7 -- not an asteroid (will add it to exclusion list)
02:27:32.20 +57:08:35.3 -- not an asteroid (will add it to exclusion list)
02:20:13.03 +56:15:34.8 -- not an asteroid (will add it to exclusion list)
02:22:27.81 +56:33:28.7 -- not an asteroid (will add it to exclusion list)
02:27:58.93 +57:31:01.3 -- not an asteroid (will add it to exclusion list)
02:33:32.05 +57:51:40.8 -- not an asteroid (will add it to exclusion list)
02:34:38.40 +57:44:07.3 -- not an asteroid (will add it to exclusion list)
02:25:47.88 +56:43:23.2 -- not an asteroid (will add it to exclusion list)
02:30:08.47 +57:20:50.2 -- not an asteroid (will add it to exclusion list)
02:38:25.27 +58:17:31.8 -- not an asteroid (will add it to exclusion list)
02:38:01.91 +58:25:43.4 -- not an asteroid (will add it to exclusion list)
02:22:07.92 +56:28:58.2 -- not an asteroid (will add it to exclusion list)
02:34:18.98 +56:07:35.1 -- not an asteroid (will add it to exclusion list)
02:27:20.09 +56:49:46.3 -- not an asteroid (will add it to exclusion list)
02:28:36.20 +56:28:40.0 -- not an asteroid (will add it to exclusion list)
02:23:45.93 +56:58:54.6 -- not an asteroid (will add it to exclusion list)
02:28:30.00 +56:31:48.6 -- not an asteroid (will add it to exclusion list)
02:28:30.82 +57:06:37.8 -- not an asteroid (will add it to exclusion list)
02:25:01.45 +56:33:15.8 -- not an asteroid (will add it to exclusion list)
02:30:19.39 +57:30:27.0 -- not an asteroid (will add it to exclusion list)
02:33:38.71 +57:12:31.9 -- not an asteroid (will add it to exclusion list)
02:32:02.17 +57:26:35.5 -- not an asteroid (will add it to exclusion list)
02:33:09.48 +57:50:43.7 -- not an asteroid (will add it to exclusion list)
02:24:54.81 +56:34:32.0 -- not an asteroid (will add it to exclusion list)
02:24:12.77 +56:08:04.7 -- not an asteroid (will add it to exclusion list)
02:24:25.62 +56:20:53.3 -- not an asteroid (will add it to exclusion list)
02:31:40.18 +57:12:25.9 -- not an asteroid (will add it to exclusion list)
02:21:22.21 +56:42:51.2 -- not an asteroid (will add it to exclusion list)
02:32:03.60 +57:19:01.2 -- not an asteroid (will add it to exclusion list)
02:29:35.90 +56:47:29.8 -- not an asteroid (will add it to exclusion list)
00:45:31.36 +61:20:32.6 -- not an asteroid (will add it to exclusion list)
02:24:19.17 +56:16:19.6 -- not an asteroid (will add it to exclusion list)
02:21:10.37 +56:34:16.2 -- not an asteroid (will add it to exclusion list)
02:25:03.41 +56:05:16.2 -- not an asteroid (will add it to exclusion list)
02:31:07.14 +56:54:53.9 -- not an asteroid (will add it to exclusion list)
02:29:01.50 +57:51:35.8 -- not an asteroid (will add it to exclusion list)
02:35:08.92 +57:20:11.7 -- not an asteroid (will add it to exclusion list)
02:38:11.28 +57:54:13.4 -- not an asteroid (will add it to exclusion list)
02:28:13.34 +57:23:00.9 -- not an asteroid (will add it to exclusion list)
01:31:48.44 +64:21:56.3 -- not an asteroid (will add it to exclusion list)
01:19:41.78 +62:51:03.2 -- not an asteroid (will add it to exclusion list)
02:37:45.34 +58:30:48.3 -- not an asteroid (will add it to exclusion list)
02:35:39.23 +57:45:01.8 -- not an asteroid (will add it to exclusion list)
01:38:33.81 +60:47:25.6 -- not an asteroid (will add it to exclusion list)
02:35:28.55 +57:41:15.0 -- not an asteroid (will add it to exclusion list)
02:24:51.53 +56:15:26.9 -- not an asteroid (will add it to exclusion list)
02:26:24.74 +56:14:06.4 -- not an asteroid (will add it to exclusion list)
02:19:14.48 +56:36:18.0 -- not an asteroid (will add it to exclusion list)
01:31:48.60 +64:22:28.2 -- not an asteroid (will add it to exclusion list)
02:32:01.89 +57:03:30.5 -- not an asteroid (will add it to exclusion list)
02:32:59.26 +57:53:54.0 -- not an asteroid (will add it to exclusion list)
02:38:06.09 +59:06:42.5 -- not an asteroid (will add it to exclusion list)
02:15:35.85 +56:21:36.3 -- not an asteroid (will add it to exclusion list)
02:38:02.06 +58:50:39.8 -- not an asteroid (will add it to exclusion list)
02:25:13.30 +56:30:31.2 -- not an asteroid (will add it to exclusion list)
02:05:05.77 +58:16:23.4 -- not an asteroid (will add it to exclusion list)
02:32:25.11 +58:26:07.8 -- not an asteroid (will add it to exclusion list)
02:33:34.78 +57:08:52.6 -- not an asteroid (will add it to exclusion list)
01:27:44.41 +62:06:39.4 -- not an asteroid (will add it to exclusion list)
01:41:47.10 +59:03:46.9 -- not an asteroid (will add it to exclusion list)
02:19:16.67 +59:42:21.1 -- not an asteroid (will add it to exclusion list)
01:39:32.69 +64:53:03.9 -- not an asteroid (will add it to exclusion list)
02:14:25.04 +56:42:47.8 -- not an asteroid (will add it to exclusion list)
02:20:07.53 +56:21:00.9 -- not an asteroid (will add it to exclusion list)
02:19:48.00 +56:25:10.7 -- not an asteroid (will add it to exclusion list)
02:34:13.06 +56:03:48.9 -- not an asteroid (will add it to exclusion list)
02:22:56.71 +57:11:44.4 -- not an asteroid (will add it to exclusion list)
02:25:27.49 +56:21:40.8 -- not an asteroid (will add it to exclusion list)
02:18:24.84 +58:37:26.7 -- not an asteroid (will add it to exclusion list)
02:23:49.27 +56:41:24.8 -- not an asteroid (will add it to exclusion list)
02:34:03.25 +56:00:34.3 -- not an asteroid (will add it to exclusion list)
01:49:47.70 +65:03:21.5 -- not an asteroid (will add it to exclusion list)
01:43:36.46 +58:48:08.2 -- not an asteroid (will add it to exclusion list)
02:38:48.34 +57:57:34.8 -- not an asteroid (will add it to exclusion list)
01:24:30.70 +59:38:48.0 -- not an asteroid (will add it to exclusion list)
02:27:22.11 +62:38:26.1 -- not an asteroid (will add it to exclusion list)
02:21:26.42 +57:16:57.3 -- not an asteroid (will add it to exclusion list)
02:27:55.31 +56:27:24.0 -- not an asteroid (will add it to exclusion list)
02:43:44.96 +60:25:27.3 -- not an asteroid (will add it to exclusion list)
02:33:40.23 +57:40:02.3 -- not an asteroid (will add it to exclusion list)
02:17:25.67 +57:06:42.6 -- not an asteroid (will add it to exclusion list)
02:37:50.78 +57:54:15.9 -- not an asteroid (will add it to exclusion list)
02:32:22.33 +58:28:54.9 -- not an asteroid (will add it to exclusion list)
02:21:36.06 +57:03:37.7 -- not an asteroid (will add it to exclusion list)
01:33:44.53 +60:46:20.5 -- not an asteroid (will add it to exclusion list)
00:53:38.56 +65:00:02.2 -- not an asteroid (will add it to exclusion list)
02:02:57.28 +62:23:12.1 -- not an asteroid (will add it to exclusion list)
02:31:45.85 +55:57:57.7 -- not an asteroid (will add it to exclusion list)
02:17:01.95 +56:44:19.3 -- not an asteroid (will add it to exclusion list)
01:52:19.58 +57:19:07.2 -- not an asteroid (will add it to exclusion list)
02:49:56.76 +63:51:39.5 -- not an asteroid (will add it to exclusion list)
02:29:48.78 +57:57:50.6 -- not an asteroid (will add it to exclusion list)
02:31:31.28 +57:22:45.9 -- not an asteroid (will add it to exclusion list)
01:43:45.33 +58:23:44.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:30:29.66 +66:05:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:54.99 +62:40:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:55.91 +62:32:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:39.91 +62:15:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:47.78 +61:53:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:31.36 +61:20:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:00.34 +57:56:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:11.73 +59:43:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:54.55 +59:03:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:55.06 +58:28:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:53:38.56 +65:00:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:55:16.01 +57:59:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:47.59 +60:38:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:58:55.93 +58:04:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:00:19.87 +57:17:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:20.28 +57:02:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:29.49 +57:06:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:39.11 +60:32:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:39.59 +63:12:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:28.97 +60:14:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:48.39 +57:17:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:14.29 +61:44:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:04.47 +60:02:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:41.78 +62:51:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:30.70 +59:38:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:15.63 +64:40:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:44.41 +62:06:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:32.95 +61:46:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:48.44 +64:21:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:48.60 +64:22:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:44.53 +60:46:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:33.81 +60:47:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:32.69 +64:53:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:01.08 +60:52:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:47.10 +59:03:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:54.46 +61:13:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:21.66 +56:52:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:36.46 +58:48:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:45.33 +58:23:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:47.70 +65:03:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:19.58 +57:19:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:38.09 +59:15:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:25.08 +60:33:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:16.63 +59:38:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:42.41 +63:32:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:56.21 +56:37:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:17.31 +65:03:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:32.89 +65:05:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:57.28 +62:23:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:05.77 +58:16:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:06.43 +63:06:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:25.04 +56:42:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:53.05 +64:11:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:35.85 +56:21:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:52.43 +56:18:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:17:01.95 +56:44:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:17:25.67 +57:06:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:17:41.08 +56:28:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:17:47.56 +56:14:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:17:50.40 +56:22:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:01.26 +56:15:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:05.24 +56:15:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:24.03 +56:23:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:24.84 +58:37:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:48.49 +56:17:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:52.86 +63:06:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:56.21 +56:18:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:14.48 +56:36:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:16.67 +59:42:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:36.20 +56:23:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:36.43 +56:14:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:39.63 +56:20:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:40.58 +56:48:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:45.01 +56:50:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:45.17 +56:31:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:45.19 +57:01:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:46.68 +56:22:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:48.00 +56:25:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:48.61 +56:23:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:52.93 +56:15:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:56.52 +56:13:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:07.36 +56:27:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:07.53 +56:21:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:11.71 +56:22:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:13.03 +56:15:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:18.71 +56:31:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:23.58 +56:22:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:24.56 +56:41:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:25.25 +56:52:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:32.11 +56:10:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:35.00 +57:06:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:50.58 +57:20:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:52.81 +56:09:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:54.08 +56:16:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:54.28 +56:36:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:55.04 +56:23:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:04.75 +56:15:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:07.65 +56:13:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:10.37 +56:34:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:13.54 +56:28:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:16.36 +56:23:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:19.11 +56:38:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:20.53 +56:29:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:22.21 +56:42:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:26.42 +57:16:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:27.44 +56:16:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:30.49 +57:12:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:33.10 +56:13:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:34.57 +56:26:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:35.29 +56:14:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:36.06 +57:03:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:36.86 +56:40:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:38.53 +56:26:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:39.29 +56:31:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:40.72 +60:54:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:50.33 +56:34:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:52.12 +56:41:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:52.46 +56:32:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:54.94 +56:42:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:55.06 +56:20:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:55.20 +56:25:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:55.92 +56:44:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:59.09 +56:30:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:03.76 +56:31:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:04.60 +57:10:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:06.90 +56:07:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:07.92 +56:28:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:10.20 +56:24:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:11.95 +56:20:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:16.04 +56:22:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:21.43 +56:34:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:22.77 +56:40:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:27.17 +56:43:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:27.81 +56:33:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:27.95 +56:41:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:29.14 +56:32:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:31.56 +56:14:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:35.38 +56:18:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:37.79 +56:37:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:47.76 +56:11:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:51.67 +56:24:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:53.49 +56:47:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:56.71 +57:11:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:02.19 +56:30:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:07.47 +56:41:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:07.87 +56:29:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:08.48 +56:20:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:11.37 +56:11:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:14.27 +56:52:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:17.91 +56:42:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:18.87 +57:06:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:26.41 +56:06:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:29.57 +56:10:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:35.48 +56:34:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:38.00 +56:52:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:38.21 +56:39:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:42.88 +56:07:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:43.00 +56:38:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:44.10 +56:55:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:45.93 +56:58:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:46.82 +57:05:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:48.03 +56:47:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:49.27 +56:41:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:53.85 +56:39:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:54.58 +56:06:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:55.73 +56:44:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:57.17 +56:11:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:57.26 +57:12:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:02.04 +56:49:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:06.49 +56:29:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:09.74 +56:34:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:11.88 +56:35:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:12.53 +56:49:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:12.77 +56:08:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:18.81 +56:54:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:18.84 +56:19:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:19.17 +56:16:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:21.26 +56:52:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:23.45 +56:13:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:23.74 +56:54:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:25.62 +56:20:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:25.89 +56:32:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:27.20 +56:50:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:29.35 +56:34:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:29.85 +59:24:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:32.13 +56:43:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:32.63 +57:00:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:33.46 +56:57:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:34.14 +56:53:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:37.23 +56:45:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:38.20 +56:49:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:38.41 +56:48:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:38.57 +56:20:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:42.01 +56:55:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:43.66 +56:59:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:46.87 +56:38:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:47.99 +56:36:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:51.53 +56:15:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:52.38 +56:43:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:53.93 +56:08:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:54.07 +56:55:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:54.81 +56:34:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:54.82 +56:45:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:58.44 +56:50:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:00.78 +56:51:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:01.45 +56:33:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:01.82 +56:15:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:03.15 +56:56:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:03.41 +56:05:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:04.29 +56:13:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:05.47 +56:20:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:07.44 +56:14:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:11.80 +56:17:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:12.20 +56:44:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:13.30 +56:30:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:20.40 +56:12:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:20.48 +56:51:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:27.49 +56:21:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:27.60 +56:46:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:28.19 +56:11:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:30.12 +56:16:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:32.87 +56:32:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:33.89 +56:34:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:39.55 +56:48:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:40.03 +56:29:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:42.31 +56:37:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:45.49 +56:26:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:45.87 +56:22:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:47.88 +56:43:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:48.30 +56:35:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:48.43 +56:32:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:48.44 +56:55:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:52.54 +57:02:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:52.96 +56:47:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:53.52 +56:14:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:54.13 +56:38:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:54.98 +56:55:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:56.01 +56:58:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:56.42 +57:04:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:56.53 +56:32:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:56.75 +56:07:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:00.84 +56:46:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:01.02 +56:28:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:02.37 +56:20:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:07.35 +56:25:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:08.97 +56:16:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:10.21 +56:21:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:10.79 +56:48:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:11.70 +56:56:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:13.46 +56:36:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:14.40 +56:12:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:15.82 +56:04:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:20.11 +57:00:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:24.74 +56:14:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:36.42 +56:34:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:43.23 +56:24:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:45.86 +56:23:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:55.66 +56:28:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:55.75 +56:30:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:58.18 +56:22:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:59.49 +57:14:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:07.72 +56:33:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:18.72 +56:15:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:20.09 +56:49:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:22.03 +56:50:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:22.05 +56:31:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:22.11 +62:38:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:23.12 +56:19:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:24.28 +56:17:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:24.37 +56:23:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:27.07 +56:31:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:31.55 +56:30:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:32.20 +57:08:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:33.11 +56:13:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:34.40 +56:16:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:39.78 +57:06:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:40.70 +56:20:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:42.18 +56:12:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:44.66 +56:19:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:48.55 +57:05:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:52.28 +56:29:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:53.71 +57:06:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:55.31 +56:27:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:57.88 +56:22:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:58.93 +57:31:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:59.53 +56:29:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:01.17 +56:23:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:09.05 +56:38:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:13.34 +57:23:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:28.47 +58:25:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:30.00 +56:31:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:30.82 +57:06:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:32.01 +56:00:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:33.48 +62:03:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:36.20 +56:28:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:44.08 +57:00:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:48.05 +56:30:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:50.69 +56:20:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:01.50 +57:51:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:08.36 +57:12:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:09.04 +56:37:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:10.13 +56:27:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:11.28 +57:21:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:17.13 +57:14:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:25.87 +55:58:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:26.34 +57:23:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:28.55 +56:33:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:29.43 +57:10:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:33.00 +55:57:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:35.90 +56:47:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:39.11 +56:11:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:41.54 +56:37:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:46.73 +56:03:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:48.78 +56:41:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:48.78 +57:57:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:55.64 +56:55:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:57.33 +56:36:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:00.34 +57:28:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:03.83 +56:36:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:07.17 +56:30:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:08.47 +57:20:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:09.68 +57:23:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:11.98 +57:38:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:16.92 +56:38:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:17.43 +56:43:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:19.30 +55:54:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:19.39 +57:30:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:30.83 +57:30:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:32.25 +57:11:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:33.01 +56:53:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:33.48 +56:57:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:35.00 +56:43:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:39.48 +57:13:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:44.95 +56:56:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:45.41 +57:06:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:51.42 +57:16:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:51.81 +57:15:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:51.91 +57:04:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:53.15 +56:59:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:55.12 +57:08:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:58.33 +57:16:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:58.90 +62:01:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:00.30 +56:00:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:02.85 +57:42:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:03.43 +55:52:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:07.14 +56:54:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:09.75 +57:16:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:10.54 +57:30:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:12.06 +57:09:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:12.57 +57:00:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:18.70 +55:53:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:18.74 +57:03:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:18.77 +57:16:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:19.72 +56:52:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:20.24 +57:33:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:20.63 +56:50:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:25.89 +56:07:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:26.00 +55:59:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:29.32 +57:11:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:31.28 +57:22:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:33.36 +57:25:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:38.55 +57:13:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:40.18 +57:12:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:45.84 +57:14:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:45.85 +55:57:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:47.11 +55:52:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:51.45 +56:45:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:52.57 +56:53:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:56.68 +57:24:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:01.27 +56:51:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:01.41 +55:53:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:01.89 +57:03:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:02.17 +57:26:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:03.60 +57:19:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:04.83 +56:49:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:04.94 +56:53:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:05.73 +57:22:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:06.03 +57:05:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:14.18 +55:56:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:17.85 +57:17:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:22.33 +58:28:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:23.31 +57:38:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:24.99 +57:27:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:25.11 +58:26:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:34.58 +57:29:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:35.29 +57:32:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:45.26 +57:08:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:47.65 +57:14:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:49.40 +57:34:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:54.63 +57:10:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:55.48 +57:08:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:58.19 +57:38:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:59.26 +57:53:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:01.74 +57:02:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:03.26 +57:03:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:03.94 +57:33:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:08.29 +57:28:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:08.50 +57:21:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:09.10 +57:00:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:09.48 +57:50:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:10.59 +57:32:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:11.11 +57:33:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:18.10 +57:31:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:27.67 +57:14:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:30.94 +57:29:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:32.05 +57:51:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:33.71 +57:37:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:34.12 +55:49:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:34.41 +56:11:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:34.76 +55:54:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:34.78 +57:08:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:37.69 +57:40:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:38.71 +57:12:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:40.23 +57:40:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:40.71 +57:26:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:43.78 +57:36:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:44.27 +56:59:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:48.55 +57:01:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:49.02 +55:57:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:49.40 +57:35:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:51.00 +55:59:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:54.63 +57:40:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:00.78 +57:49:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:03.25 +56:00:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:04.49 +57:32:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:04.61 +57:19:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:10.54 +55:50:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:12.97 +56:11:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:13.06 +56:03:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:13.94 +56:18:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:18.98 +56:07:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:19.87 +57:08:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:24.39 +57:28:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:31.90 +56:11:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:31.90 +57:40:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:35.60 +57:34:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:38.40 +57:44:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:38.93 +57:26:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:41.26 +56:11:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:42.72 +57:17:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:44.20 +56:06:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:44.93 +57:54:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:46.00 +58:00:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:46.10 +57:12:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:46.52 +57:13:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:48.66 +57:38:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:04.64 +57:26:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:08.67 +57:36:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:08.92 +57:20:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:18.48 +57:31:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:20.24 +57:29:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:26.60 +57:46:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:28.55 +57:41:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:34.92 +57:32:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:37.82 +57:29:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:39.23 +57:45:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:41.37 +57:27:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:42.02 +57:31:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:52.03 +57:47:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:58.35 +57:49:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:58.93 +57:32:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:02.71 +59:00:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:07.79 +57:32:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:08.52 +57:39:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:12.26 +57:41:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:17.73 +57:48:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:22.58 +57:40:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:25.89 +57:52:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:33.27 +57:54:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:35.03 +57:36:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:36.22 +57:46:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:41.37 +57:37:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:55.81 +57:38:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:59.45 +57:56:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:01.15 +57:51:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:02.20 +57:41:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:12.84 +63:10:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:15.58 +57:48:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:36.88 +57:51:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:45.34 +58:30:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:47.78 +57:52:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:50.64 +57:45:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:50.68 +57:57:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:50.78 +57:54:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:52.11 +57:47:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:58.92 +58:07:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:01.91 +58:25:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:02.06 +58:50:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:06.09 +59:06:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:11.28 +57:54:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:13.42 +57:50:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:14.42 +57:58:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:19.87 +58:03:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:25.27 +58:17:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:46.76 +57:49:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:48.34 +57:57:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:39:21.42 +58:07:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:39:23.99 +58:09:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:39:52.21 +58:24:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:43:44.96 +60:25:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:49:56.76 +63:51:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:52:02.80 +63:39:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:52:09.97 +62:49:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:30:29.66 +66:05:42.3 -- not a known variable star
00:36:54.99 +62:40:45.5 -- not a known variable star
00:36:55.91 +62:32:56.0 -- not a known variable star
00:37:39.91 +62:15:59.9 -- not a known variable star
00:43:47.78 +61:53:59.7 -- not a known variable star
00:45:31.36 +61:20:32.6 -- not a known variable star
00:46:00.34 +57:56:20.1 -- not a known variable star
00:46:11.73 +59:43:33.6 -- not a known variable star
00:47:54.55 +59:03:26.0 -- a known variable star
00:52:55.06 +58:28:52.6 -- not a known variable star
00:53:38.56 +65:00:02.2 -- not a known variable star
00:55:16.01 +57:59:06.5 -- not a known variable star
00:56:47.59 +60:38:47.2 -- not a known variable star
00:58:55.93 +58:04:05.2 -- not a known variable star
01:00:19.87 +57:17:48.3 -- not a known variable star
01:02:20.28 +57:02:48.2 -- not a known variable star
01:08:29.49 +57:06:54.4 -- not a known variable star
01:08:39.11 +60:32:48.4 -- not a known variable star
01:13:39.59 +63:12:31.2 -- not a known variable star
01:16:28.97 +60:14:00.3 -- a known variable star
01:17:48.39 +57:17:35.2 -- not a known variable star
01:18:14.29 +61:44:36.0 -- not a known variable star
01:19:04.47 +60:02:34.1 -- not a known variable star
01:19:41.78 +62:51:03.2 -- not a known variable star
01:24:30.70 +59:38:48.0 -- a known variable star
01:25:15.63 +64:40:33.5 -- not a known variable star
01:27:44.41 +62:06:39.4 -- a known variable star
01:29:32.95 +61:46:25.0 -- not a known variable star
01:31:48.44 +64:21:56.3 -- not a known variable star
01:31:48.60 +64:22:28.2 -- not a known variable star
01:33:44.53 +60:46:20.5 -- not a known variable star
01:38:33.81 +60:47:25.6 -- not a known variable star
01:39:32.69 +64:53:03.9 -- a known variable star
01:40:01.08 +60:52:38.4 -- not a known variable star
01:41:47.10 +59:03:46.9 -- a known variable star
01:42:54.46 +61:13:30.6 -- not a known variable star
01:43:21.66 +56:52:28.8 -- not a known variable star
01:43:36.46 +58:48:08.2 -- a known variable star
01:43:45.33 +58:23:44.8 -- a known variable star
01:49:47.70 +65:03:21.5 -- a known variable star
01:52:19.58 +57:19:07.2 -- a known variable star
01:56:38.09 +59:15:33.9 -- a known variable star
01:57:25.08 +60:33:52.9 -- a known variable star
01:58:16.63 +59:38:57.1 -- not a known variable star
01:59:42.41 +63:32:29.7 -- not a known variable star
01:59:56.21 +56:37:09.2 -- not a known variable star
02:00:17.31 +65:03:54.9 -- not a known variable star
02:01:32.89 +65:05:48.8 -- not a known variable star
02:02:57.28 +62:23:12.1 -- a known variable star
02:05:05.77 +58:16:23.4 -- a known variable star
02:08:06.43 +63:06:02.0 -- not a known variable star
02:14:25.04 +56:42:47.8 -- not a known variable star
02:14:53.05 +64:11:56.5 -- not a known variable star
02:15:35.85 +56:21:36.3 -- not a known variable star
02:16:52.43 +56:18:43.8 -- not a known variable star
02:17:01.95 +56:44:19.3 -- not a known variable star
02:17:25.67 +57:06:42.6 -- a known variable star
02:17:41.08 +56:28:32.5 -- not a known variable star
02:17:47.56 +56:14:45.2 -- not a known variable star
02:17:50.40 +56:22:37.9 -- not a known variable star
02:18:01.26 +56:15:41.5 -- not a known variable star
02:18:05.24 +56:15:07.5 -- not a known variable star
02:18:24.03 +56:23:21.4 -- not a known variable star
02:18:24.84 +58:37:26.7 -- a known variable star
02:18:48.49 +56:17:54.8 -- a known variable star
02:18:52.86 +63:06:09.6 -- not a known variable star
02:18:56.21 +56:18:32.0 -- not a known variable star
02:19:14.48 +56:36:18.0 -- not a known variable star
02:19:16.67 +59:42:21.1 -- a known variable star
02:19:36.20 +56:23:21.9 -- a known variable star
02:19:36.43 +56:14:20.7 -- not a known variable star
02:19:39.63 +56:20:11.8 -- not a known variable star
02:19:40.58 +56:48:52.6 -- not a known variable star
02:19:45.01 +56:50:30.5 -- not a known variable star
02:19:45.17 +56:31:44.3 -- not a known variable star
02:19:45.19 +57:01:14.5 -- not a known variable star
02:19:46.68 +56:22:26.5 -- not a known variable star
02:19:48.00 +56:25:10.7 -- not a known variable star
02:19:48.61 +56:23:45.9 -- not a known variable star
02:19:52.93 +56:15:40.7 -- not a known variable star
02:19:56.52 +56:13:26.0 -- not a known variable star
02:20:07.36 +56:27:52.1 -- not a known variable star
02:20:07.53 +56:21:00.9 -- not a known variable star
02:20:11.71 +56:22:22.8 -- a known variable star
02:20:13.03 +56:15:34.8 -- not a known variable star
02:20:18.71 +56:31:49.5 -- a known variable star
02:20:23.58 +56:22:39.7 -- not a known variable star
02:20:24.56 +56:41:43.6 -- a known variable star
02:20:25.25 +56:52:28.8 -- a known variable star
02:20:32.11 +56:10:00.6 -- not a known variable star
02:20:35.00 +57:06:52.7 -- a known variable star
02:20:50.58 +57:20:41.9 -- a known variable star
02:20:52.81 +56:09:33.8 -- a known variable star
02:20:54.08 +56:16:37.4 -- a known variable star
02:20:54.28 +56:36:05.4 -- not a known variable star
02:20:55.04 +56:23:19.2 -- a known variable star
02:21:04.75 +56:15:32.3 -- a known variable star
02:21:07.65 +56:13:22.2 -- a known variable star
02:21:10.37 +56:34:16.2 -- not a known variable star
02:21:13.54 +56:28:44.7 -- not a known variable star
02:21:16.36 +56:23:43.0 -- not a known variable star
02:21:19.11 +56:38:13.4 -- not a known variable star
02:21:20.53 +56:29:12.7 -- not a known variable star
02:21:22.21 +56:42:51.2 -- not a known variable star
02:21:26.42 +57:16:57.3 -- not a known variable star
02:21:27.44 +56:16:28.6 -- not a known variable star
02:21:30.49 +57:12:34.5 -- a known variable star
02:21:33.10 +56:13:41.1 -- not a known variable star
02:21:34.57 +56:26:43.9 -- not a known variable star
02:21:35.29 +56:14:56.5 -- not a known variable star
02:21:36.06 +57:03:37.7 -- not a known variable star
02:21:36.86 +56:40:52.1 -- not a known variable star
02:21:38.53 +56:26:50.2 -- a known variable star
02:21:39.29 +56:31:44.8 -- a known variable star
02:21:40.72 +60:54:41.9 -- a known variable star
02:21:50.33 +56:34:31.6 -- not a known variable star
02:21:52.12 +56:41:17.7 -- not a known variable star
02:21:52.46 +56:32:45.3 -- not a known variable star
02:21:54.94 +56:42:38.7 -- not a known variable star
02:21:55.06 +56:20:50.1 -- not a known variable star
02:21:55.20 +56:25:08.5 -- not a known variable star
02:21:55.92 +56:44:53.0 -- a known variable star
02:21:59.09 +56:30:01.6 -- a known variable star
02:22:03.76 +56:31:27.4 -- not a known variable star
02:22:04.60 +57:10:38.0 -- a known variable star
02:22:06.90 +56:07:52.9 -- a known variable star
02:22:07.92 +56:28:58.2 -- not a known variable star
02:22:10.20 +56:24:23.3 -- not a known variable star
02:22:11.95 +56:20:47.3 -- not a known variable star
02:22:16.04 +56:22:42.6 -- not a known variable star
02:22:21.43 +56:34:19.1 -- not a known variable star
02:22:22.77 +56:40:00.7 -- not a known variable star
02:22:27.17 +56:43:56.9 -- a known variable star
02:22:27.81 +56:33:28.7 -- not a known variable star
02:22:27.95 +56:41:51.9 -- a known variable star
02:22:29.14 +56:32:00.5 -- not a known variable star
02:22:31.56 +56:14:10.7 -- a known variable star
02:22:35.38 +56:18:13.9 -- not a known variable star
02:22:37.79 +56:37:17.0 -- not a known variable star
02:22:47.76 +56:11:09.8 -- not a known variable star
02:22:51.67 +56:24:33.0 -- not a known variable star
02:22:53.49 +56:47:13.1 -- a known variable star
02:22:56.71 +57:11:44.4 -- not a known variable star
02:23:02.19 +56:30:28.6 -- not a known variable star
02:23:07.47 +56:41:44.4 -- not a known variable star
02:23:07.87 +56:29:01.2 -- not a known variable star
02:23:08.48 +56:20:24.9 -- not a known variable star
02:23:11.37 +56:11:21.3 -- not a known variable star
02:23:14.27 +56:52:06.4 -- not a known variable star
02:23:17.91 +56:42:23.9 -- a known variable star
02:23:18.87 +57:06:02.1 -- not a known variable star
02:23:26.41 +56:06:42.3 -- not a known variable star
02:23:29.57 +56:10:15.1 -- not a known variable star
02:23:35.48 +56:34:27.4 -- a known variable star
02:23:38.00 +56:52:44.8 -- not a known variable star
02:23:38.21 +56:39:53.8 -- not a known variable star
02:23:42.88 +56:07:10.8 -- not a known variable star
02:23:43.00 +56:38:37.8 -- not a known variable star
02:23:44.10 +56:55:56.9 -- not a known variable star
02:23:45.93 +56:58:54.6 -- not a known variable star
02:23:46.82 +57:05:04.4 -- not a known variable star
02:23:48.03 +56:47:01.5 -- not a known variable star
02:23:49.27 +56:41:24.8 -- not a known variable star
02:23:53.85 +56:39:14.7 -- not a known variable star
02:23:54.58 +56:06:52.8 -- a known variable star
02:23:55.73 +56:44:45.5 -- not a known variable star
02:23:57.17 +56:11:53.7 -- not a known variable star
02:23:57.26 +57:12:24.5 -- not a known variable star
02:24:02.04 +56:49:22.3 -- not a known variable star
02:24:06.49 +56:29:59.8 -- not a known variable star
02:24:09.74 +56:34:02.3 -- not a known variable star
02:24:11.88 +56:35:43.2 -- not a known variable star
02:24:12.53 +56:49:25.8 -- not a known variable star
02:24:12.77 +56:08:04.7 -- not a known variable star
02:24:18.81 +56:54:02.0 -- a known variable star
02:24:18.84 +56:19:49.3 -- not a known variable star
02:24:19.17 +56:16:19.6 -- not a known variable star
02:24:21.26 +56:52:14.7 -- a known variable star
02:24:23.45 +56:13:56.3 -- a known variable star
02:24:23.74 +56:54:04.6 -- not a known variable star
02:24:25.62 +56:20:53.3 -- not a known variable star
02:24:25.89 +56:32:55.3 -- not a known variable star
02:24:27.20 +56:50:28.9 -- not a known variable star
02:24:29.35 +56:34:20.6 -- not a known variable star
02:24:29.85 +59:24:31.1 -- a known variable star
02:24:32.13 +56:43:35.2 -- not a known variable star
02:24:32.63 +57:00:44.1 -- a known variable star
02:24:33.46 +56:57:18.3 -- not a known variable star
02:24:34.14 +56:53:00.2 -- not a known variable star
02:24:37.23 +56:45:53.9 -- not a known variable star
02:24:38.20 +56:49:55.7 -- not a known variable star
02:24:38.41 +56:48:43.1 -- a known variable star
02:24:38.57 +56:20:45.4 -- not a known variable star
02:24:42.01 +56:55:47.8 -- not a known variable star
02:24:43.66 +56:59:33.7 -- not a known variable star
02:24:46.87 +56:38:55.3 -- not a known variable star
02:24:47.99 +56:36:57.6 -- a known variable star
02:24:51.53 +56:15:26.9 -- not a known variable star
02:24:52.38 +56:43:10.9 -- not a known variable star
02:24:53.93 +56:08:45.2 -- not a known variable star
02:24:54.07 +56:55:39.8 -- a known variable star
02:24:54.81 +56:34:32.0 -- not a known variable star
02:24:54.82 +56:45:04.1 -- not a known variable star
02:24:58.44 +56:50:40.4 -- not a known variable star
02:25:00.78 +56:51:31.9 -- not a known variable star
02:25:01.45 +56:33:15.8 -- not a known variable star
02:25:01.82 +56:15:07.5 -- not a known variable star
02:25:03.15 +56:56:58.8 -- not a known variable star
02:25:03.41 +56:05:16.2 -- a known variable star
02:25:04.29 +56:13:07.5 -- not a known variable star
02:25:05.47 +56:20:33.3 -- not a known variable star
02:25:07.44 +56:14:04.5 -- not a known variable star
02:25:11.80 +56:17:22.8 -- not a known variable star
02:25:12.20 +56:44:30.7 -- not a known variable star
02:25:13.30 +56:30:31.2 -- not a known variable star
02:25:20.40 +56:12:12.7 -- not a known variable star
02:25:20.48 +56:51:13.6 -- not a known variable star
02:25:27.49 +56:21:40.8 -- not a known variable star
02:25:27.60 +56:46:56.1 -- not a known variable star
02:25:28.19 +56:11:20.2 -- not a known variable star
02:25:30.12 +56:16:52.8 -- a known variable star
02:25:32.87 +56:32:57.7 -- not a known variable star
02:25:33.89 +56:34:21.9 -- not a known variable star
02:25:39.55 +56:48:00.4 -- a known variable star
02:25:40.03 +56:29:20.6 -- not a known variable star
02:25:42.31 +56:37:12.9 -- a known variable star
02:25:45.49 +56:26:32.2 -- not a known variable star
02:25:45.87 +56:22:47.0 -- a known variable star
02:25:47.88 +56:43:23.2 -- not a known variable star
02:25:48.30 +56:35:16.7 -- not a known variable star
02:25:48.43 +56:32:35.4 -- a known variable star
02:25:48.44 +56:55:12.4 -- not a known variable star
02:25:52.54 +57:02:04.3 -- not a known variable star
02:25:52.96 +56:47:30.0 -- not a known variable star
02:25:53.52 +56:14:35.6 -- not a known variable star
02:25:54.13 +56:38:48.5 -- a known variable star
02:25:54.98 +56:55:26.7 -- not a known variable star
02:25:56.01 +56:58:59.2 -- not a known variable star
02:25:56.42 +57:04:40.2 -- not a known variable star
02:25:56.53 +56:32:31.9 -- not a known variable star
02:25:56.75 +56:07:50.5 -- not a known variable star
02:26:00.84 +56:46:18.0 -- not a known variable star
02:26:01.02 +56:28:14.9 -- a known variable star
02:26:02.37 +56:20:59.5 -- not a known variable star
02:26:07.35 +56:25:11.7 -- not a known variable star
02:26:08.97 +56:16:06.3 -- a known variable star
02:26:10.21 +56:21:10.3 -- not a known variable star
02:26:10.79 +56:48:28.8 -- not a known variable star
02:26:11.70 +56:56:03.6 -- not a known variable star
02:26:13.46 +56:36:46.9 -- not a known variable star
02:26:14.40 +56:12:13.5 -- not a known variable star
02:26:15.82 +56:04:34.0 -- not a known variable star
02:26:20.11 +57:00:45.6 -- not a known variable star
02:26:24.74 +56:14:06.4 -- not a known variable star
02:26:36.42 +56:34:16.7 -- not a known variable star
02:26:43.23 +56:24:12.4 -- not a known variable star
02:26:45.86 +56:23:26.2 -- a known variable star
02:26:55.66 +56:28:24.5 -- not a known variable star
02:26:55.75 +56:30:20.2 -- not a known variable star
02:26:58.18 +56:22:12.1 -- a known variable star
02:26:59.49 +57:14:44.2 -- a known variable star
02:27:07.72 +56:33:53.0 -- not a known variable star
02:27:18.72 +56:15:53.5 -- a known variable star
02:27:20.09 +56:49:46.3 -- a known variable star
02:27:22.03 +56:50:16.1 -- a known variable star
02:27:22.05 +56:31:18.8 -- a known variable star
02:27:22.11 +62:38:26.1 -- a known variable star
02:27:23.12 +56:19:27.5 -- a known variable star
02:27:24.28 +56:17:59.4 -- not a known variable star
02:27:24.37 +56:23:03.5 -- a known variable star
02:27:27.07 +56:31:10.2 -- not a known variable star
02:27:31.55 +56:30:00.3 -- not a known variable star
02:27:32.20 +57:08:35.3 -- a known variable star
02:27:33.11 +56:13:09.8 -- not a known variable star
02:27:34.40 +56:16:53.2 -- not a known variable star
02:27:39.78 +57:06:42.3 -- not a known variable star
02:27:40.70 +56:20:28.5 -- not a known variable star
02:27:42.18 +56:12:19.8 -- not a known variable star
02:27:44.66 +56:19:43.0 -- not a known variable star
02:27:48.55 +57:05:55.3 -- a known variable star
02:27:52.28 +56:29:28.8 -- not a known variable star
02:27:53.71 +57:06:30.9 -- not a known variable star
02:27:55.31 +56:27:24.0 -- a known variable star
02:27:57.88 +56:22:23.8 -- not a known variable star
02:27:58.93 +57:31:01.3 -- not a known variable star
02:27:59.53 +56:29:42.2 -- not a known variable star
02:28:01.17 +56:23:28.1 -- not a known variable star
02:28:09.05 +56:38:21.2 -- not a known variable star
02:28:13.34 +57:23:00.9 -- not a known variable star
02:28:28.47 +58:25:05.6 -- not a known variable star
02:28:30.00 +56:31:48.6 -- not a known variable star
02:28:30.82 +57:06:37.8 -- not a known variable star
02:28:32.01 +56:00:36.5 -- not a known variable star
02:28:33.48 +62:03:22.8 -- not a known variable star
02:28:36.20 +56:28:40.0 -- not a known variable star
02:28:44.08 +57:00:25.5 -- not a known variable star
02:28:48.05 +56:30:07.8 -- not a known variable star
02:28:50.69 +56:20:49.6 -- not a known variable star
02:29:01.50 +57:51:35.8 -- not a known variable star
02:29:08.36 +57:12:16.0 -- not a known variable star
02:29:09.04 +56:37:12.3 -- not a known variable star
02:29:10.13 +56:27:12.4 -- not a known variable star
02:29:11.28 +57:21:01.0 -- not a known variable star
02:29:17.13 +57:14:30.0 -- not a known variable star
02:29:25.87 +55:58:55.7 -- a known variable star
02:29:26.34 +57:23:02.8 -- a known variable star
02:29:28.55 +56:33:06.0 -- a known variable star
02:29:29.43 +57:10:39.0 -- not a known variable star
02:29:33.00 +55:57:16.1 -- not a known variable star
02:29:35.90 +56:47:29.8 -- not a known variable star
02:29:39.11 +56:11:33.0 -- a known variable star
02:29:41.54 +56:37:30.7 -- not a known variable star
02:29:46.73 +56:03:52.6 -- not a known variable star
02:29:48.78 +56:41:55.8 -- not a known variable star
02:29:48.78 +57:57:50.6 -- not a known variable star
02:29:55.64 +56:55:49.6 -- not a known variable star
02:29:57.33 +56:36:50.4 -- not a known variable star
02:30:00.34 +57:28:19.7 -- not a known variable star
02:30:03.83 +56:36:39.2 -- a known variable star
02:30:07.17 +56:30:20.8 -- a known variable star
02:30:08.47 +57:20:50.2 -- not a known variable star
02:30:09.68 +57:23:15.1 -- not a known variable star
02:30:11.98 +57:38:18.7 -- not a known variable star
02:30:16.92 +56:38:09.4 -- not a known variable star
02:30:17.43 +56:43:02.2 -- a known variable star
02:30:19.30 +55:54:55.0 -- not a known variable star
02:30:19.39 +57:30:27.0 -- not a known variable star
02:30:30.83 +57:30:27.8 -- not a known variable star
02:30:32.25 +57:11:26.3 -- not a known variable star
02:30:33.01 +56:53:09.2 -- not a known variable star
02:30:33.48 +56:57:02.6 -- not a known variable star
02:30:35.00 +56:43:58.4 -- not a known variable star
02:30:39.48 +57:13:42.2 -- not a known variable star
02:30:44.95 +56:56:12.6 -- not a known variable star
02:30:45.41 +57:06:28.3 -- not a known variable star
02:30:51.42 +57:16:48.8 -- not a known variable star
02:30:51.81 +57:15:44.6 -- not a known variable star
02:30:51.91 +57:04:09.8 -- not a known variable star
02:30:53.15 +56:59:21.2 -- not a known variable star
02:30:55.12 +57:08:07.5 -- not a known variable star
02:30:58.33 +57:16:17.2 -- not a known variable star
02:30:58.90 +62:01:46.4 -- not a known variable star
02:31:00.30 +56:00:28.1 -- not a known variable star
02:31:02.85 +57:42:08.9 -- not a known variable star
02:31:03.43 +55:52:01.6 -- not a known variable star
02:31:07.14 +56:54:53.9 -- not a known variable star
02:31:09.75 +57:16:14.4 -- not a known variable star
02:31:10.54 +57:30:46.6 -- a known variable star
02:31:12.06 +57:09:47.8 -- not a known variable star
02:31:12.57 +57:00:49.3 -- not a known variable star
02:31:18.70 +55:53:50.8 -- not a known variable star
02:31:18.74 +57:03:50.9 -- a known variable star
02:31:18.77 +57:16:22.0 -- not a known variable star
02:31:19.72 +56:52:39.5 -- not a known variable star
02:31:20.24 +57:33:46.4 -- not a known variable star
02:31:20.63 +56:50:06.3 -- a known variable star
02:31:25.89 +56:07:05.1 -- not a known variable star
02:31:26.00 +55:59:07.0 -- a known variable star
02:31:29.32 +57:11:54.7 -- not a known variable star
02:31:31.28 +57:22:45.9 -- not a known variable star
02:31:33.36 +57:25:43.5 -- not a known variable star
02:31:38.55 +57:13:46.4 -- not a known variable star
02:31:40.18 +57:12:25.9 -- not a known variable star
02:31:45.84 +57:14:33.1 -- a known variable star
02:31:45.85 +55:57:57.7 -- not a known variable star
02:31:47.11 +55:52:28.5 -- not a known variable star
02:31:51.45 +56:45:51.1 -- a known variable star
02:31:52.57 +56:53:49.0 -- not a known variable star
02:31:56.68 +57:24:00.2 -- not a known variable star
02:32:01.27 +56:51:17.5 -- not a known variable star
02:32:01.41 +55:53:20.2 -- not a known variable star
02:32:01.89 +57:03:30.5 -- not a known variable star
02:32:02.17 +57:26:35.5 -- not a known variable star
02:32:03.60 +57:19:01.2 -- not a known variable star
02:32:04.83 +56:49:24.9 -- not a known variable star
02:32:04.94 +56:53:51.4 -- not a known variable star
02:32:05.73 +57:22:03.4 -- not a known variable star
02:32:06.03 +57:05:00.6 -- not a known variable star
02:32:14.18 +55:56:22.8 -- a known variable star
02:32:17.85 +57:17:09.3 -- a known variable star
02:32:22.33 +58:28:54.9 -- not a known variable star
02:32:23.31 +57:38:37.3 -- not a known variable star
02:32:24.99 +57:27:18.3 -- not a known variable star
02:32:25.11 +58:26:07.8 -- not a known variable star
02:32:34.58 +57:29:15.3 -- not a known variable star
02:32:35.29 +57:32:20.9 -- not a known variable star
02:32:45.26 +57:08:08.0 -- not a known variable star
02:32:47.65 +57:14:17.2 -- a known variable star
02:32:49.40 +57:34:21.9 -- not a known variable star
02:32:54.63 +57:10:57.1 -- not a known variable star
02:32:55.48 +57:08:54.0 -- not a known variable star
02:32:58.19 +57:38:43.0 -- not a known variable star
02:32:59.26 +57:53:54.0 -- a known variable star
02:33:01.74 +57:02:07.9 -- a known variable star
02:33:03.26 +57:03:29.0 -- not a known variable star
02:33:03.94 +57:33:09.8 -- not a known variable star
02:33:08.29 +57:28:10.5 -- a known variable star
02:33:08.50 +57:21:20.2 -- not a known variable star
02:33:09.10 +57:00:38.5 -- not a known variable star
02:33:09.48 +57:50:43.7 -- not a known variable star
02:33:10.59 +57:32:53.7 -- a known variable star
02:33:11.11 +57:33:48.8 -- not a known variable star
02:33:18.10 +57:31:36.8 -- not a known variable star
02:33:27.67 +57:14:45.0 -- not a known variable star
02:33:30.94 +57:29:02.8 -- a known variable star
02:33:32.05 +57:51:40.8 -- not a known variable star
02:33:33.71 +57:37:46.7 -- not a known variable star
02:33:34.12 +55:49:25.9 -- not a known variable star
02:33:34.41 +56:11:48.0 -- a known variable star
02:33:34.76 +55:54:25.0 -- not a known variable star
02:33:34.78 +57:08:52.6 -- not a known variable star
02:33:37.69 +57:40:25.1 -- not a known variable star
02:33:38.71 +57:12:31.9 -- not a known variable star
02:33:40.23 +57:40:02.3 -- not a known variable star
02:33:40.71 +57:26:09.7 -- not a known variable star
02:33:43.78 +57:36:02.2 -- not a known variable star
02:33:44.27 +56:59:34.7 -- not a known variable star
02:33:48.55 +57:01:45.9 -- not a known variable star
02:33:49.02 +55:57:06.8 -- not a known variable star
02:33:49.40 +57:35:12.5 -- a known variable star
02:33:51.00 +55:59:56.1 -- not a known variable star
02:33:54.63 +57:40:55.2 -- not a known variable star
02:34:00.78 +57:49:58.1 -- not a known variable star
02:34:03.25 +56:00:34.3 -- not a known variable star
02:34:04.49 +57:32:44.3 -- not a known variable star
02:34:04.61 +57:19:27.3 -- not a known variable star
02:34:10.54 +55:50:00.3 -- a known variable star
02:34:12.97 +56:11:54.0 -- not a known variable star
02:34:13.06 +56:03:48.9 -- not a known variable star
02:34:13.94 +56:18:42.0 -- not a known variable star
02:34:18.98 +56:07:35.1 -- not a known variable star
02:34:19.87 +57:08:33.3 -- not a known variable star
02:34:24.39 +57:28:26.1 -- not a known variable star
02:34:31.90 +56:11:08.8 -- not a known variable star
02:34:31.90 +57:40:30.4 -- not a known variable star
02:34:35.60 +57:34:23.2 -- not a known variable star
02:34:38.40 +57:44:07.3 -- not a known variable star
02:34:38.93 +57:26:15.3 -- not a known variable star
02:34:41.26 +56:11:01.6 -- not a known variable star
02:34:42.72 +57:17:58.8 -- a known variable star
02:34:44.20 +56:06:07.0 -- not a known variable star
02:34:44.93 +57:54:58.3 -- not a known variable star
02:34:46.00 +58:00:26.7 -- not a known variable star
02:34:46.10 +57:12:52.3 -- not a known variable star
02:34:46.52 +57:13:22.5 -- not a known variable star
02:34:48.66 +57:38:04.9 -- not a known variable star
02:35:04.64 +57:26:52.9 -- not a known variable star
02:35:08.67 +57:36:14.5 -- not a known variable star
02:35:08.92 +57:20:11.7 -- not a known variable star
02:35:18.48 +57:31:39.8 -- not a known variable star
02:35:20.24 +57:29:29.9 -- not a known variable star
02:35:26.60 +57:46:11.7 -- not a known variable star
02:35:28.55 +57:41:15.0 -- not a known variable star
02:35:34.92 +57:32:59.3 -- not a known variable star
02:35:37.82 +57:29:13.2 -- not a known variable star
02:35:39.23 +57:45:01.8 -- a known variable star
02:35:41.37 +57:27:01.8 -- not a known variable star
02:35:42.02 +57:31:40.9 -- a known variable star
02:35:52.03 +57:47:22.2 -- not a known variable star
02:35:58.35 +57:49:15.3 -- a known variable star
02:35:58.93 +57:32:00.1 -- not a known variable star
02:36:02.71 +59:00:55.3 -- not a known variable star
02:36:07.79 +57:32:58.9 -- not a known variable star
02:36:08.52 +57:39:33.9 -- not a known variable star
02:36:12.26 +57:41:56.0 -- a known variable star
02:36:17.73 +57:48:52.1 -- not a known variable star
02:36:22.58 +57:40:05.6 -- not a known variable star
02:36:25.89 +57:52:58.9 -- not a known variable star
02:36:33.27 +57:54:38.9 -- not a known variable star
02:36:35.03 +57:36:36.2 -- not a known variable star
02:36:36.22 +57:46:58.9 -- not a known variable star
02:36:41.37 +57:37:08.5 -- not a known variable star
02:36:55.81 +57:38:49.8 -- not a known variable star
02:36:59.45 +57:56:29.8 -- a known variable star
02:37:01.15 +57:51:23.0 -- not a known variable star
02:37:02.20 +57:41:39.3 -- not a known variable star
02:37:12.84 +63:10:37.8 -- a known variable star
02:37:15.58 +57:48:19.2 -- not a known variable star
02:37:36.88 +57:51:16.7 -- not a known variable star
02:37:45.34 +58:30:48.3 -- a known variable star
02:37:47.78 +57:52:43.0 -- not a known variable star
02:37:50.64 +57:45:49.7 -- not a known variable star
02:37:50.68 +57:57:56.9 -- not a known variable star
02:37:50.78 +57:54:15.9 -- not a known variable star
02:37:52.11 +57:47:13.1 -- a known variable star
02:37:58.92 +58:07:38.9 -- a known variable star
02:38:01.91 +58:25:43.4 -- not a known variable star
02:38:02.06 +58:50:39.8 -- not a known variable star
02:38:06.09 +59:06:42.5 -- not a known variable star
02:38:11.28 +57:54:13.4 -- a known variable star
02:38:13.42 +57:50:16.2 -- not a known variable star
02:38:14.42 +57:58:50.6 -- not a known variable star
02:38:19.87 +58:03:56.7 -- not a known variable star
02:38:25.27 +58:17:31.8 -- not a known variable star
02:38:46.76 +57:49:57.1 -- not a known variable star
02:38:48.34 +57:57:34.8 -- not a known variable star
02:39:21.42 +58:07:09.8 -- not a known variable star
02:39:23.99 +58:09:11.5 -- not a known variable star
02:39:52.21 +58:24:37.9 -- not a known variable star
02:43:44.96 +60:25:27.3 -- a known variable star
02:49:56.76 +63:51:39.5 -- not a known variable star
02:52:02.80 +63:39:30.2 -- not a known variable star
02:52:09.97 +62:49:57.4 -- not a known variable star
Found 392 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
503 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 503 (excluding asteroids and hot pixels, 392 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461199.83116492 -observatory V36
06:44:34.58 +24:58:32.7 Mercury (0.1mag)
07:43:33.48 +23:21:06.4 Venus (-4.0mag)
02:50:01.03 +15:44:43.8 Mars (1.3mag)
07:48:33.23 +21:31:09.3 Jupiter (-1.9mag)
00:49:24.87 +02:48:53.9 Saturn (0.9mag)
04:00:14.42 +20:25:33.4 Uranus (5.8mag)
00:16:09.05 +00:16:51.0 Neptune (7.8mag)
20:33:20.95 -23:04:36.0 Pluto (14.5mag)
23:10:17.71 -04:53:05.5 Moon (-10.4mag)
-rw-r--r-- 1 apache apache 362 Jun 8 03:10 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461199.83116492:
07:48:37.54 +21:30:58.5 Io (6.0mag)
07:48:36.20 +21:31:02.6 Europa (6.2mag)
07:48:17.25 +21:31:57.7 Ganymede (5.6mag)
07:48:50.52 +21:30:13.0 Callisto (6.7mag)
07:48:50.10 +21:07:27.6 Himalia (15.6mag)
07:48:35.61 +21:31:01.5 Thebe (16.5mag)
07:48:49.31 +21:22:50.4 Elara (17.5mag)
07:50:44.37 +21:42:46.6 Pasiphae (17.7mag)
07:55:07.96 +21:32:52.4 Carme (18.9mag)
00:49:15.73 +02:48:51.1 Titan (8.7mag)
00:49:21.19 +02:49:05.7 Rhea (9.9mag)
00:49:57.06 +02:51:04.1 Iapetus (11.3mag)
00:49:21.34 +02:48:30.0 Hyperion (14.7mag)
00:50:06.95 +02:50:49.2 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 8 03:10 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461199.83116492:
17:26:00.68 -35:17:32.9 JWST
15:17:25.63 +54:00:04.4 Chandra
20:42:41.09 +37:00:04.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 8 03:10 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461199.83116492 -observatory V36
18:43:24.88 -32:39:51.3 13.6mag P/2010 H2 (Vales)
05:53:36.41 -68:03:45.2 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:49:06.61 +31:58:11.2 17.5mag C/2017 K2 (PANSTARRS)
17:14:40.58 +15:21:31.8 17.8mag C/2021 G2 (ATLAS)
21:13:31.54 -49:25:30.9 16.9mag P/2021 N1 (ZTF)
23:12:36.24 +31:35:50.7 17.2mag C/2022 E2 (ATLAS)
05:34:12.68 +26:58:34.6 16.5mag C/2022 N2 (PANSTARRS)
09:29:49.57 +31:04:39.9 16.6mag C/2022 QE78 (ATLAS)
08:50:37.17 +03:56:18.7 17.7mag C/2022 R6 (PANSTARRS)
18:28:07.95 +21:36:18.2 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:19:19.37 -11:00:31.8 17.6mag P/2023 B1 (PANSTARRS)
22:14:23.27 +66:32:14.3 17.7mag C/2023 H5 (Lemmon)
17:46:02.86 -06:42:09.3 13.7mag C/2023 R1 (PANSTARRS)
13:18:00.98 +82:57:43.5 17.9mag C/2023 X2 (Lemmon)
07:10:36.36 +64:18:48.5 17.7mag C/2024 A1 (ATLAS)
06:47:28.84 +27:50:47.3 13.6mag C/2024 E1 (Wierzchos)
15:37:10.83 +13:32:18.3 17.4mag C/2024 G6 (ATLAS)
20:12:57.30 +31:10:34.8 14.0mag C/2024 J3 (ATLAS)
04:18:09.86 -15:56:20.5 16.0mag C/2024 T5 (ATLAS)
06:06:02.43 +34:28:03.5 17.9mag C/2025 J1 (Borisov)
11:34:50.26 +52:44:26.9 17.4mag C/2025 L1 (ATLAS)
06:45:06.83 -10:52:33.2 14.1mag C/2025 R3 (PANSTARRS)
09:24:16.41 +23:20:17.1 17.9mag C/2025 V2 (Rankin)
12:39:41.82 +04:41:26.2 17.2mag C/2025 Y1 (ATLAS)
18:12:39.82 +75:09:44.6 17.9mag C/2026 A2 (Bok)
02:00:54.37 +43:25:31.1 16.1mag C/2026 B2 (Sun-Gao)
11:11:20.35 -03:41:05.9 16.5mag A/2026 E1
20:23:53.63 -08:34:46.3 8.7mag 10P/Tempel
11:02:02.21 -00:58:11.7 16.0mag 29P/Schwassmann-Wachmann
03:11:56.05 +25:39:50.6 17.7mag 47P/Ashbrook-Jackson
09:00:16.34 +23:43:47.6 16.9mag 63P/Wild
00:27:02.75 -06:21:31.4 15.7mag 65P/Gunn
06:43:53.13 +33:26:37.0 16.9mag 76P/West-Kohoutek-Ikemura
03:09:30.82 +17:14:03.1 13.8mag 78P/Gehrels
01:21:03.52 +04:52:45.0 15.6mag 88P/Howell
04:55:05.00 +30:18:48.0 15.3mag 93P/Lovas
02:43:20.36 +27:38:53.2 17.6mag 114P/Wiseman-Skiff
06:50:52.50 +33:01:59.2 15.6mag 123P/West-Hartley
09:50:25.00 +14:34:43.5 16.5mag 124P/Mrkos
03:59:15.76 +19:15:34.7 16.4mag 128P/Shoemaker-Holt
04:33:50.24 +19:05:26.8 17.7mag 131P/Mueller
05:58:54.08 +18:38:58.4 14.7mag 141P/Machholz
06:01:32.70 +17:40:56.7 14.6mag 141P-A/Machholz
04:54:46.92 +16:11:32.9 11.6mag 141P-D/Machholz
02:57:46.62 -24:40:50.4 16.8mag 161P/Hartley-IRAS
03:41:59.94 +23:51:52.0 14.9mag 162P/SidingSpring
19:36:37.20 +01:46:10.2 16.9mag 169P/NEAT
00:18:42.38 +02:29:32.0 17.9mag 220P/McNaught
16:52:04.41 -08:28:08.9 16.4mag 235P/LINEAR
07:34:58.04 +35:29:09.7 17.5mag 240P/NEAT
00:32:42.68 -02:24:40.2 16.4mag 260P/McNaught
04:04:35.87 +32:30:21.2 17.6mag 295P/LINEAR
23:53:08.55 -09:32:11.2 17.6mag 320P/McNaught
15:15:10.50 +08:05:42.6 17.4mag 391P/Kowalski
08:07:14.76 +20:44:37.7 17.9mag 450P/LONEOS
07:00:11.81 +41:41:12.0 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 8 03:10 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
-rw-r--r-- 1 apache apache 5.6K Jun 8 03:10 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
-rw-r--r-- 1 apache apache 189K Jun 8 03:10 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:39:35.110 +15:17:58.28 AT 2026nsc 2026-05-09.80 20.76
16:42:48.680 +20:27:18.30 AT 2026nsb 2026-05-09.80 20.54
13:34:03.440 +31:37:31.73 AT 2026nsa 2026-05-07.80 21.26
13:50:28.150 +02:34:54.72 AT 2026nrz 2026-05-22.72 21.54
13:43:59.750 +03:47:21.63 AT 2026nry 2026-05-22.69 22.05
13:17:26.150 -01:26:00.12 AT 2026nrx 2026-05-21.64 21.7
00:35:20.216 -08:28:38.64 AT 2026nrw 2026-05-19.42 18.74
23:50:43.016 -01:09:12.25 AT 2026nrv 2026-05-23.48 19.5028
22:36:47.715 +37:31:34.81 AT 2026nru 2026-05-22.43 19.4626
23:58:04.247 +20:56:44.66 AT 2026nrt 2026-05-23.48 20.1237
16:08:58.229 +36:53:23.76 AT 2026nrs 2026-05-21.36 20.3819
19:44:04.734 +84:44:44.91 SN 2026nrr 2026-05-25.47 17.808
21:42:24.388 -20:21:08.51 SN 2026nrq 2026-05-25.56 18.623
22:03:20.669 -84:55:27.45 AT 2026nrp 2026-05-22.30 19.244
23:07:53.376 -39:04:26.84 AT 2026nro 2026-05-22.38 19.567
00:40:07.848 -39:10:21.32 AT 2026nrn 2026-05-12.41 18.737
23:05:28.381 -21:25:50.28 AT 2026nrm 2026-05-25.58 18.887
19:27:28.750 -48:42:52.35 AT 2026nrl 2026-05-22.24 19.107
12:33:38.422 +12:02:05.88 AT 2026nrk 2026-05-25.29 21.322
12:32:27.199 +02:39:54.51 AT 2026nrj 2026-05-25.29 21.0728
-rw-r--r-- 1 apache apache 30K Jun 8 03:10 tns_transients_list.txt
